The galaxy presents a largely smooth, elliptical morphology. Its overall shape is predominantly round, with only a slight deviation towards an elongated form. There is no discernible spiral arm structure or bar feature visible. The light distribution is concentrated toward the center, indicating the presence of a central bulge. The galaxy appears relatively isolated and does not exhibit any signs of major interaction or tidal disturbance with nearby galaxies. Its color profile suggests a population of older stars. There might be some minor disturbances, but this is not a merging event. The object could be classified as a giant elliptical galaxy, but further analysis would be required.