The galaxy exhibits a generally elliptical morphology. Its light is concentrated towards the center, with a bright, smooth nucleus. The color gradient suggests an older stellar population dominating, with the light appearing more reddish-orange. There is little evidence of strong spiral arm structure or significant dust lanes. The edges of the galaxy appear diffuse and fade gradually into the background sky, making it difficult to precisely define its outer boundaries. Overall, the galaxy appears to be relatively undisturbed, with no obvious signs of ongoing major mergers or tidal interactions.
