This galaxy presents as a relatively smooth, centrally concentrated object. It appears to be elliptical in shape, displaying an axis ratio suggesting a moderate degree of flattening. The central region exhibits a bright, compact core, likely indicative of a significant stellar population or possible active galactic nucleus, though further spectral analysis would be required to confirm the latter. Surrounding the core is a more diffuse halo that fades gradually into the background. The color profile suggests a population dominated by older stars, evidenced by the overall redder hue, although a subtle bluer component indicates the possibility of recent or ongoing star formation activity, particularly in the outer regions of the galaxy. There is no apparent evidence of strong tidal features or major disturbances, indicating that it has not undergone a major merger in the recent past, though minor disturbances are possible. Overall, this galaxy presents as a fairly evolved system, potentially transitioning from active star formation to a more quiescent state.
