This galaxy exhibits a primarily smooth morphology, with a bright central region that is slightly elongated in shape. The core appears to be dominated by a concentrated distribution of stars, possibly indicating an older stellar population. There is evidence of a surrounding disk component, seen as a fainter, more diffuse structure extending outwards from the central bulge. The disk appears relatively undisturbed, with no strong spiral arm structures readily visible. The overall color of the galaxy suggests a mix of stellar ages, with the central region appearing slightly yellower (likely older stars) and the outer disk showing hints of bluer colors (potentially younger stars or regions of ongoing star formation). There is a subtle distortion in the outer regions of the galaxy that indicates a possible minor gravitational interaction. The tidal feature could be a result of either a past or ongoing merger event. The structure is complex. Further analysis of the color gradients across the galaxy would be needed to assess the star formation history and the distribution of stellar populations.
