The galaxy presents as a relatively smooth, elliptical structure. It exhibits a concentrated central bulge that is bright yellow/white. The outer regions of the galaxy fade in intensity, displaying a reddish hue that suggests an older stellar population. There is no evidence of spiral arms or prominent dust lanes. The overall form indicates a generally relaxed system with no major mergers or significant disturbances readily apparent. The galaxy's elongated shape lies somewhere between round and cigar-shaped. No significant star forming regions can be observed.
