The galaxy presents as a centrally concentrated, smooth, and relatively round object. It displays a yellowish-white hue, which might indicate an older stellar population. No spiral arm structures or prominent dust lanes are discernible. There may be a slight asymmetry or minor disturbance in the outer regions, but it appears largely undisturbed. Overall, the galaxy's morphology suggests a lack of ongoing major merging activity. Its relatively compact size and smooth appearance point towards a likely elliptical or lenticular classification. The subdued colors are consistent with low levels of current star formation.
