The galaxy presents as a generally smooth object with an elliptical morphology. There is some evidence of a faint disk-like structure or spiral arms within the galaxy, though it is not well-defined. The galaxy's light distribution is relatively concentrated, with a brighter central region and a gradual decrease in brightness toward the outer edges. Color indices suggest the presence of a significant population of older stars, as well as the presence of ongoing star formation. The galaxy shows minor disturbances, suggesting recent or ongoing interactions or mergers.
