The galaxy presents as a generally elliptical form, exhibiting a smooth, diffuse light distribution with a high degree of central concentration. Its color is a relatively uniform yellowish-white, suggesting a stellar population dominated by older stars. There is little evidence of spiral arms or significant dust lanes. The morphology appears largely undisturbed, with no obvious signs of tidal interactions or ongoing mergers. The slight elongation present suggests a nearly circular shape. Overall, the galaxy seems to be a relatively evolved system, likely an elliptical galaxy, with a relatively quiescent star formation history.
