The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology appears to be largely spheroidal. The galaxy exhibits a pronounced central bulge, characterized by a yellowish hue, suggestive of an older stellar population. The outer regions of the galaxy show a gradual decline in brightness, with a slightly bluer color, possibly indicating the presence of younger stars or some ongoing star formation activity, though it seems minimal. There is no clear evidence of a prominent disk structure or spiral arms in this image. The overall shape appears mostly round, with no strong tidal features or indications of a major ongoing merger event. There might be some minor asymmetries or disturbances in the outer regions, suggesting past interactions or minor mergers.
