The galaxy appears to be a relatively compact, elliptical galaxy with a smooth, diffuse light profile. It exhibits a slight elongation, approaching a cigar-like shape, suggesting some degree of asymmetry. The color profile indicates a concentration of older stellar populations toward the center, as evidenced by the yellowish-orange hue, while bluer, younger stars appear to be sparse. There is no distinct spiral arm structure or dust lane visible. There are faint, less distinct appendages to the top of the galaxy that could potentially be the beginning of a minor disturbance of some kind. Overall, the galaxy seems to be relatively isolated and quiescent, with a high likelihood of being a spheroidal system with a significant fraction of its stars already formed.
