The galaxy presents a generally smooth, elliptical morphology. Its core is bright and concentrated, with a gradual decrease in luminosity moving outwards. There is some indication of a possible disk or faint feature extending horizontally. The galaxy displays a color gradient, appearing bluer near the feature and more reddish towards the center, suggesting a mix of stellar populations with older stars concentrated in the bulge. Based on its round shape, it is likely an elliptical galaxy. There does not appear to be evidence of any major recent merger events, though some minor disturbances are not entirely ruled out, as the profile is not perfectly smooth.
