The galaxy appears as a slightly elongated, centrally concentrated object. Its overall morphology suggests a smooth, spheroid-dominated system, likely an elliptical galaxy or a lenticular galaxy viewed at a moderate inclination. The light distribution is relatively uniform, with a gradual decrease in intensity from the core outwards, indicating an absence of prominent spiral arms or strong bar structures. The galaxy's color profile is suggestive of an older stellar population, with a yellowish-red hue that implies the presence of evolved stars and relatively low ongoing star formation. No distinct dust lanes or prominent star-forming regions are discernible within the galaxy's body. There is no visible evidence of major ongoing mergers or tidal disturbances. The galaxy's overall symmetry and smooth light profile point towards a system that has likely undergone significant dynamical relaxation.
