The galaxy presents as a relatively smooth, elliptical structure, with a concentrated central bulge. A slight elongation is observed, although it appears nearly circular. The overall color is bluish-white, possibly indicating the presence of a younger stellar population and ongoing star formation, although at a low rate. There is no evidence of spiral arms or a distinct disk component. No obvious signs of a major merger event are visible, with only minor disturbances being possible. The galaxy appears relatively isolated in its environment based on the lack of other objects in close proximity.
