The galaxy presents as a centrally concentrated, relatively smooth structure. The overall morphology appears largely elliptical, with a high degree of central light concentration. There is a suggestion of a slight ellipticity, but the galaxy appears mostly round from this viewing angle. Color gradients are subtle; however, the central region exhibits a whiter appearance, potentially indicating an older stellar population. A faint, diffuse halo may be present but is not clearly defined. There's no obvious presence of distinct spiral arms or significant dust lanes. The galaxy does not show any strong signs of ongoing star formation. There is a very subtle distortion which suggests it is undergoing a minor merger.
