The galaxy presents as a generally smooth, elliptical-like structure. It appears to be relatively undisturbed, without any signs of a major merger or tidal disruptions. The galaxy is fairly symmetrical, exhibiting a spheroidal shape with a high degree of roundness. A slight color gradient is observable; the central region is bright with a possible change in hue, potentially indicating a difference in stellar population or dust content compared to the outer regions. The overall color suggests the presence of older stellar populations. The faintness of the outer regions indicates a lower density of stars as one moves away from the core. No obvious spiral arms, bar structures, or prominent dust lanes are detected.
