The galaxy presents an elliptical morphology, appearing largely smooth and featureless in its overall structure. A concentrated central bulge dominates the visual impression, exhibiting a yellowish-orange hue indicative of an older stellar population. The light gradually fades towards the outer regions of the galaxy, showing a slight greenish tint in the periphery. The lack of distinct spiral arms or prominent dust lanes suggests a classification toward the early-type end of the Hubble sequence. There is no evidence of major mergers or tidal disturbances that would significantly disrupt its smooth appearance. A minor disturbance may be present. The light distribution indicates a moderate size for the galaxy.
