The galaxy appears to be a relatively smooth, centrally concentrated object. Its overall shape is elliptical, tending towards a rounder morphology. There is a noticeable color gradient, with the central region exhibiting a yellowish-orange hue, potentially indicating an older stellar population. Fainter bluish tones are present in the outer regions. There is no evidence of distinct spiral arms, a prominent bar, or ongoing major mergers. Subtle asymmetries or minor disturbances cannot be ruled out.
