This galaxy presents as a relatively smooth and centrally concentrated object. It appears elliptical in shape, with a bright, diffuse core that gradually fades into the surrounding halo. There is little evidence of significant spiral arm structure or prominent dust lanes. The overall color is somewhat redder, suggesting an older stellar population, although hints of blue indicate the presence of some younger stars and ongoing star formation. There may be a slight perturbation or minor asymmetry visible on one side, potentially indicative of a minor interaction, but no major disturbances or signs of a major merger are apparent.
