The galaxy appears as a relatively smooth, elliptical structure. It exhibits a concentrated central bulge that dominates its overall light distribution, surrounded by a more diffuse halo. The galaxy presents a yellowish color, which suggests a population of older stars and a low rate of ongoing star formation. No distinct spiral arms or prominent dust lanes are discernible, reinforcing the classification of this object as elliptical. The galaxy has moderate size. There is no obvious evidence of a major ongoing merger, but there is a slight asymmetry in the outer regions.
