The galaxy presents as a relatively smooth, elliptical morphology. The central region exhibits a concentrated luminosity, appearing nearly spherical, with a slight elongation along one axis, transitioning toward a cigar-shaped form, though the rounding is clearly in between round and cigar-shaped. There are no obvious spiral arms or significant disk-like structures visible. The galaxy appears to be generally undisturbed, with no prominent signs of a recent major merger event. Faint features of minor disturbances may be present in the outer regions, but are not distinct. Color gradients are apparent, with the core exhibiting a yellowish/reddish hue, suggestive of an older stellar population. The outer regions display a bluer tint, possibly indicating the presence of younger stars, but these are not prominent. The overall smooth appearance indicates that the rate of star formation is relatively low.
