The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a roughly elliptical morphology, appearing more elongated than circular, but not excessively so. A prominent central bulge region dominates the luminosity profile, appearing bright and somewhat yellowish. Fainter, bluer extended features are visible surrounding the central bulge, giving the impression of a faint, diffuse disk. There is some indication of a slight disturbance in the galaxy's morphology, potentially suggesting a minor interaction or past merger event. This may be causing asymmetry in the faint disk. Overall, the galaxy appears to be a mature system with ongoing but low levels of star formation.
