This galaxy presents as a system with at least two distinct components or nuclei. The overall morphology appears relatively smooth and rounded. The primary component exhibits a concentrated, bright central region that transitions outward to a more diffuse halo. This main component displays a yellowish-white hue, potentially indicating a population of older stars. Adjacent to the primary object is a secondary component, slightly less luminous but similar in color. There is indication of possible tidal features or interactions between the two components, although the resolution is not high enough to confirm this. The overall system shows little evidence of strong spiral arm structures or significant star formation activity. The general shape appears relatively undisturbed, though the presence of multiple nuclei suggests a possible ongoing or recent merger event.
