The galaxy presents as a smooth, elliptical-like structure. It exhibits a concentrated central bulge with a notable decrease in luminosity towards its outer regions. The galaxy appears to be relatively undisturbed with no obvious signs of recent major mergers or tidal interactions. Its overall color is slightly redder, suggesting a population dominated by older stars and a relatively low rate of current star formation. The axial ratio indicates the galaxy is moderately flattened, with the major axis oriented at an angle. While some disk like qualities could be present, the lack of spiral arms and overall smoothed appearance suggests an early-type galaxy.
