The galaxy presents as a relatively smooth, centrally concentrated object with a slightly elongated morphology. The core region exhibits a yellowish-white hue, possibly indicating an older stellar population. Fainter, bluer extensions are tentatively observed on either side of the core, suggestive of a weak disk-like structure or tidal features. A very mild disturbance is possibly evident, though no strong signs of an active merger are seen. The overall structure appears to be more elliptical than spiral.
