The galaxy appears as an elliptical-type galaxy, characterized by a generally smooth and concentrated light profile. It exhibits a slight elongation, deviating marginally from a perfectly circular morphology. The central region is noticeably brighter and more yellow, indicative of an older stellar population dominating the core. The outer regions appear to have a more blueish tint suggesting the presence of ongoing, although not significant, star formation within the galaxy's disk. There is no clear evidence of spiral arm structure or significant dust lanes. The galaxy does not appear to be undergoing any major mergers or exhibiting tidal disturbances. Overall, it seems to be a relatively undisturbed elliptical galaxy with a moderate level of star formation.
