The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. A slight elongation is visible, deviating from a perfectly circular morphology. The color profile indicates an older stellar population, with a yellowish core that likely harbors older, redder stars. Faint, diffuse blue regions are observed in the outer portions of the galaxy, possibly hinting at some ongoing, albeit weak, star formation activity within a disk like structure. There is no clear evidence of spiral arms or a bar feature. The overall smooth appearance of the galaxy suggests that it is not currently undergoing any major merging events, although some subtle asymmetry cannot be ruled out as indicative of past minor interactions. The object appears to be quite compact.
