The galaxy presents as a relatively smooth, centrally concentrated system. The light distribution suggests a spheroidal morphology, with a high degree of radial symmetry. There is little evidence of spiral arms or a prominent disk structure; instead, the galaxy appears largely featureless, with a gradual decline in surface brightness away from the center. The core region displays a slightly bluer color compared to the outer regions, which appear redder. No obvious signs of strong tidal interactions or recent major mergers are observed; however, a mild disturbance or minor interaction cannot be fully ruled out. Overall, the galaxy appears to be a relaxed system consistent with an elliptical or lenticular classification, exhibiting a low star formation rate.
