This galaxy appears to be a relatively smooth, disk-like structure, likely an elliptical or lenticular type. It exhibits a bright, concentrated central bulge that fades gradually into the surrounding disk. The overall color is dominated by light on the redder end of the spectrum, indicative of a population of older stars, although there is some evidence of bluer star formation regions, particularly within the disk and around the core. The galaxy is elongated in shape, suggesting a flattened structure with a possible bar component along its major axis. There may be slight evidence of tidal interaction or minor disturbances in the outer disk, which warrant further investigation. There are no clear signs of a major merger event in the image.
