The galaxy exhibits an elliptical morphology, presenting as a somewhat smooth, centrally concentrated object. The color gradient suggests an older stellar population, with a yellow-orange hue dominating the central bulge. There are hints of bluer, more diffuse light extending from the central region, possibly indicating regions of more recent star formation within a disk-like structure. There is no indication of strong spiral arm structure or a distinct bar feature. The galaxy appears relatively undisturbed, with no obvious signs of tidal interactions or a recent major merger.
