The galaxy presents as a relatively smooth, elliptical morphology. It exhibits a concentrated central bulge region that gradually fades outward into a less defined halo. Color gradients within the galaxy suggest a population of older stars dominating the central regions, indicated by a subtle shift towards redder hues. There's little evidence of spiral arm structure or significant dust lanes. The overall symmetry suggests it is a relaxed system without prominent signs of recent mergers or tidal disturbances.
