The galaxy presents as a disk-shaped system, observed at a relatively high inclination angle. A prominent central bulge dominates the light profile, appearing smooth and concentrated. Fainter disk components extend outwards from this central region. The light distribution suggests a spiral structure, though the arms appear somewhat flocculent and not well-defined. Patches of bluer light are visible within the disk, indicative of ongoing star formation activity. There is some evidence of minor distortions, potentially due to past interactions. Overall, the galaxy seems to be in a relatively late stage of evolution, with a significant population of older stars contributing to the redder colors of the bulge.
