The galaxy exhibits an irregular morphology. It does not present a clear spiral arm structure or elliptical shape. There are several distinct clumps of higher intensity emission, possibly indicative of active star-forming regions, scattered throughout the body of the galaxy. The distribution of light appears uneven, suggesting possible gravitational interactions or mergers in its past or ongoing.

The galaxy displays variations in color. The redder hues could indicate regions of older stellar populations or dust obscuration, while the bluer regions are likely associated with hotter, younger stars. The integrated light across the galaxy is predominantly greenish-blue. A bright, somewhat crescent-shaped structure borders part of the galaxy. Within this feature, color segregation is apparent, hinting at either a gradient in stellar populations or differential extinction. The overall structure is quite perturbed, with indications of tidal features possibly emanating from the primary body.

The galaxy's disturbed nature suggests that it may be undergoing a merger or tidal interaction, although there isn't clear evidence of a second distinct galaxy within the immediate vicinity. Higher resolution images or spectroscopic data would aid in confirming these hypotheses.
