This galaxy exhibits a primarily smooth morphology, suggesting an elliptical type. The light profile is centrally concentrated with a gradual decrease in intensity outwards, forming an elliptical shape. The core appears bright and somewhat diffuse, potentially indicating an older stellar population. There are some hints of possible minor disturbances or features within the galaxy's outer regions, such as slightly irregular isophotes, but nothing to indicate recent violent major mergers. Color gradients are subtle but visible. The central region seems to be more yellow. Hints of red knots within the galaxy suggest some ongoing star formation. Overall, this galaxy appears relatively relaxed.
