The galaxy presents a lenticular morphology, appearing as a smooth, flattened disk with minimal discernible spiral arm structure. Its orientation is nearly edge-on relative to our line of sight, which obscures any potential central bulge or bar features. The galaxy exhibits a color gradient, appearing bluer towards its outer edges, suggestive of younger stellar populations in these regions, and redder toward its center, potentially indicating older, more evolved stars. The overall color suggests intermediate activity. The disk appears relatively undisturbed, showing no obvious signs of major mergers or tidal interactions with nearby galaxies. Some faint, diffuse light extends beyond the main body of the galaxy, which may be a faint halo of older stars.
