This galaxy appears to be a relatively smooth, centrally concentrated system, characterized by a generally elliptical morphology. The central region exhibits a bright, concentrated core, indicating a significant stellar density. There is a gradual decrease in luminosity from the core outwards, blending into a more diffuse halo. There is no strong evidence of spiral arm structures or prominent dust lanes. The light appears to be yellowish/red, this suggests that the galaxy is primarily composed of an older stellar population. The galaxy appears to be relatively undisturbed, without evidence of recent major mergers or tidal interactions.
