The galaxy presents as a smooth, elliptical morphology. Its light profile is centrally concentrated with a gradual decrease in brightness moving outwards. The core region exhibits a yellowish hue, suggesting a population of older stars. There is very little evidence of spiral arm structure or dust lanes. The overall form appears to be undisturbed, showing no significant signs of tidal interactions or recent mergers, although a very faint asymmetry cannot be ruled out.
