The galaxy presents a primarily smooth morphology. There is a concentration of light towards the center, suggesting a prominent galactic bulge. The overall shape appears somewhat elliptical, though not perfectly round, and the outer regions show a gradual decrease in surface brightness. There may be faint, broad arm-like structures or tidal features present, but these are not sharply defined. The galaxy exhibits a yellow-white hue, which may indicate a population of older stars, although the presence of bluer regions suggests ongoing star formation at a low rate. There is no strong evidence of a major merger or significant tidal disruption.
