The galaxy presents a generally smooth, elliptical morphology. Its core region is highly concentrated and appears bright, emitting strongly in bluer wavelengths. This color suggests ongoing, though possibly declining, star formation in the nuclear region, or a significant population of older, blue stars. The galaxy exhibits a gradual decrease in surface brightness moving outward from the center. There are no readily discernible spiral arms or significant dust lanes. There is a subtle elongation to the overall shape, deviating slightly from a perfectly circular form. No major disturbances or interactions with other galaxies are immediately apparent, though there might be minor tidal features that require further investigation with higher resolution data. The galaxy does not display prominent active galactic nuclei (AGN) features in this optical view. Overall, it appears as a relatively quiescent, moderately sized galaxy, likely undergoing slow evolution.
