The galaxy presents as a moderately bright, somewhat diffuse object. It exhibits an elliptical morphology, with a smooth, concentrated central bulge. The color gradient suggests a population of older stars dominating the central region, indicated by a yellowish hue. The outer regions fade in brightness and display a bluer tint, possibly indicating the presence of younger stellar populations and ongoing star formation in the disk. There appears to be a slight asymmetry in the galaxy's outer regions, hinting at a possible minor gravitational interaction.
