The galaxy presents as a single, luminous entity with a generally elliptical morphology. It appears largely featureless with a smooth luminosity profile, lacking any obvious spiral arms or distinct disk structure. There is a concentration of light toward the center, which could be interpreted as a galactic bulge. The light is predominantly yellow/orange, suggesting a population of older stars. The overall symmetry is very high. No signs of tidal disturbances or ongoing mergers are evident, and the galaxy's shape appears regular and relaxed. There is a very slight indication of a fainter halo surrounding the main body of the galaxy, but the light is rather uniform.
