The galaxy presents as an elliptical morphology, appearing relatively smooth and spheroidal in shape. Its light profile suggests a concentrated central bulge with a gradual decrease in luminosity toward the outer regions, exhibiting no prominent spiral arm structures or dust lanes. The galaxy’s color index indicates a population of older stars, predominantly yellowish-red hues, suggesting a lack of significant ongoing star formation. There is a possible faint extended halo surrounding the galaxy, although it blends subtly with the background sky. There is no indication of a major merger or significant tidal disturbance in the galaxy's structure.
