The galaxy presents as a relatively smooth, centralized object with a generally elliptical morphology. There appears to be minimal or no significant visible disk structure. The color profile is broadly consistent across the galaxy's body, indicating a potentially older stellar population and subdued ongoing star formation. No signs of major mergers or significant tidal disturbances are observed. The concentration of light suggests a dominant central bulge. A slight elongation is present, without a discernible bar.
