The galaxy presents as a central, bright, relatively compact object. Its overall morphology appears disturbed.

The core is luminous, showing a concentration of light that is rather intense. Surrounding the central region, we observe some asymmetric structure. Patches of varying colors and intensities suggest active star formation, dust lanes, or areas of ionized gas. The colors suggest a higher concentration of older stars in the nucleus compared to the exterior of the galaxy. The outer regions exhibit hints of tidal features.

Evidence of a minor or major disturbance exists in the galactic structure, with no distinct spiral arms. Further analysis would be required to confirm the nature and origin of this feature.
