The galaxy appears to be a relatively smooth, centrally concentrated object. It exhibits a generally elliptical morphology, though it deviates slightly from perfect roundness. A bright, yellowish core is evident, suggesting a concentration of older stars and potentially a supermassive black hole actively accreting matter. The outer regions of the galaxy display a bluer hue compared to the core, indicating the presence of a younger stellar population and possibly ongoing star formation. There appears to be a very slight asymmetry in the light distribution, though no clear signs of major interactions or mergers with other galaxies are readily apparent. There is a faint, disk like feature around the core of the galaxy.
