The galaxy presents a smooth, elliptical morphology. It appears to be a relatively quiescent system with minimal discernible substructure, spiral arms, or dust lanes. The galaxy exhibits a concentrated central bulge, surrounded by a more diffuse halo. The color gradient transitions from a yellowish core to a slightly bluer outer region, suggestive of older stellar populations dominating the central region and younger, possibly star-forming populations present in the outskirts. The elongation indicates a potential cigar shape. There are no obvious signs of major mergers or tidal disturbances. Overall, it resembles a typical elliptical galaxy with moderate star formation occurring.
