The galaxy presents as a luminous elliptical object with a significant spheroidal component. The core region exhibits a high degree of central concentration. The light profile appears to be well-fit by a Sersic profile with a high Sersic index, indicating a centrally concentrated morphology. The galaxy displays a moderate ellipticity, appearing somewhat flattened. There is a subtle color gradient present with a predominantly red central bulge that transitions to bluer hues in the outer regions of the galaxy. This suggests a complex stellar population, with older stars dominating the center and younger stars distributed in the periphery. Faint, diffuse extensions are potentially visible along the major axis, possibly indicating tidal features or remnants of past interactions, but these are not distinctly resolved. There does not appear to be significant dust obscuration or spiral arm structure visible in this image.
