The galaxy presents an elliptical morphology. A bright, concentrated core is present, suggesting a significant population of older stars. The main body of the galaxy exhibits a smooth, diffuse texture, with a gradual decrease in luminosity extending outwards from the core. The light is more reddish than bluish. The outer edges are somewhat irregular, possibly indicating interactions or past mergers. There are no strong indications of spiral arm structures or significant dust lanes visible. The galaxy appears to be relatively inclined, presenting a flattened shape.
