The galaxy appears to be a smooth, relatively featureless elliptical. It exhibits a concentrated central bulge that dominates the structure and gradually fades into the outer regions. The galaxy is slightly elongated, presenting an intermediate shape between round and cigar-shaped. There is a color gradient visible, with the central regions exhibiting a yellowish hue, suggesting an older stellar population, transitioning to a slightly bluer color towards the periphery, which could indicate the presence of some younger stars or ongoing star formation. There is a very faint possible disturbance of the disc that could be a minor merger event. There are no clear spiral arms or prominent dust lanes visible. The overall light distribution suggests a high degree of symmetry, typical of early-type galaxies.
