The galaxy presents a morphology that appears largely smooth and elliptical in shape, with a bright central bulge. There is a subtle disk component, but it lacks well-defined spiral arms. The light distribution transitions gradually from a highly concentrated core to a more diffuse outer region. There is indication of ongoing low levels of star formation. The galaxy has an intermediate roundness, neither perfectly circular nor highly elongated. There is no strong evidence of a major ongoing merger, although subtle disturbances and minor asymmetries are present in the outer regions, which could be indicative of tidal interactions or minor mergers in its past. The galaxy displays a color gradient, with the central bulge appearing more yellow-reddish in color than the outer regions of the galaxy.
