The galaxy presents a generally smooth appearance, suggesting it may be an elliptical galaxy or a spiral galaxy viewed face-on at a considerable distance. There is a slight elongation, but the shape is largely circular. A bright, concentrated central region is observed, potentially indicating an active galactic nucleus (AGN) or a dense stellar population within the bulge. The color profile suggests a higher concentration of older stars, or a redder stellar population overall. There are faint hints of substructure, suggesting a possible minor interaction or merger in the past.
