The galaxy presents an elliptical morphology, exhibiting a smooth, centrally concentrated light distribution. The primary component displays a yellowish-orange hue, indicating a population of older stars. A secondary, smaller, and bluer component is observed adjacent to the main body. The presence of this blue component suggests ongoing or recent star formation. There is no evidence of spiral arm structure. The overall appearance implies a relatively evolved system with a possible interaction or merger event triggering localized star formation. The galaxy appears to be relatively isolated, with no immediately obvious tidal features or nearby companions.
