The galaxy appears to be an elliptical or lenticular type, exhibiting a smooth, somewhat elongated morphology. It displays a bright, centrally concentrated bulge with a diffuse halo extending outwards. Color gradients suggest the presence of older stellar populations, particularly within the bulge, indicated by its yellowish-orange hue. There is a noticeable lack of distinct spiral arm structures or prominent dust lanes, consistent with a relatively quiescent star formation rate. Its axial ratio suggests a moderate degree of flattening. There is the slight indication of minor disturbances, possibly interaction with another smaller galaxy.
