The object appears to be an elliptical galaxy with a smooth, centrally concentrated light distribution. The galaxy's morphology suggests it is relatively undisturbed, without strong tidal features or evidence of recent major mergers. It exhibits a generally elliptical shape, tending toward a slightly elongated form, and its color profile indicates an older stellar population. There is a distinct lack of resolved spiral arms or prominent dust lanes. The core region is particularly bright, suggesting a higher concentration of stars. Faint, diffuse outer regions extend some distance from the central core but lack distinct features. The overall color suggests the presence of evolved stars.
