The galaxy presents as a relatively compact object with a high degree of central concentration. A bright, yellowish core dominates the image, indicating a significant population of older stars. Moving outward from the core, a smoother, bluer halo is present, suggesting some ongoing star formation, albeit at a modest rate. The overall morphology appears generally elliptical, with no distinct spiral arm structure discernible. There are no obvious signs of major mergers or tidal disruptions, but a slight asymmetry or minor disturbance cannot be ruled out. The galaxy displays an intermediate roundness. The light distribution falls off gradually from the center, consistent with a smooth stellar population.
