The galaxy appears to be a relatively smooth, centrally concentrated object. It presents as an elliptical or lenticular galaxy, lacking prominent spiral arms or a well-defined disk structure. There is a noticeable, bright core region, surrounded by a more diffuse halo. The object shows a moderate degree of ellipticity, appearing somewhat elongated. The color profile suggests a population of older stars, exhibiting a slightly redder hue in the outer regions compared to the central bulge, which appears bluer, suggestive of some ongoing, though low, star formation. No significant tidal features or signs of major disturbance from mergers are apparent, though there is a subtle asymmetry hinting at possible minor interactions.
