The galaxy appears to be relatively compact, with a bright central core suggesting a concentration of stars or potentially an active galactic nucleus. Surrounding the core is a diffuse, asymmetrical halo of light. There is evidence of potential distortion or tidal features, indicated by the slightly irregular shape and extensions of light emanating from the main body. These features may be evidence of a minor disturbance or interaction with another galaxy.

The light distribution indicates varying stellar populations or dust content within the galaxy. The presence of redder regions suggests older stellar populations or dust obscuration, while bluer regions could indicate younger, hotter stars forming in areas of active star formation. However, the overall appearance seems relatively smooth, with no obvious spiral arms or distinct disk structures readily apparent.
