The galaxy presents as a relatively smooth, elliptical structure, with a diffuse, almost featureless morphology. It exhibits a slightly elongated shape, leaning towards an 'in-between' elliptical classification rather than perfectly round or cigar-shaped. There is a subtle color gradient visible, with the central region appearing somewhat brighter and potentially slightly redder than the outer edges, which tend toward bluer hues. The galaxy does not show any obvious signs of significant ongoing mergers or major disturbances. The overall appearance suggests a system dominated by an older stellar population, with a relatively low rate of current star formation activity.
