This galaxy exhibits an overall elliptical morphology, appearing somewhat smooth in structure. The light distribution suggests a relatively even spread of stars throughout the galactic body, with no prominent spiral arms visible. There is evidence of a slight elongation, falling between round and cigar shaped, suggesting a moderate degree of ellipticity.

Several features point to possible interactions or disturbances. There appears to be a distorted shape or tidal tail potentially indicating on going or recent galaxy merger. Areas of the galaxy show a non-uniform color distribution, perhaps indicating distinct stellar populations or regions of enhanced star formation. A possible merging event or close interaction with another galaxy is likely.
