The galaxy presents as a fairly smooth, elliptical-like object with a concentrated central bulge. The core appears bright and yellow, potentially indicating an older stellar population dominating the nuclear region. There is a faint, diffuse halo surrounding the core, extending outwards with a slight red hue. There are no visible spiral arms or significant dust lanes. The overall morphology suggests a galaxy that has largely completed its star formation, though it still possesses some capacity. There does not appear to be evidence of any major ongoing merger events, but there may be minor irregularities in the outer halo structure that hint at past interactions. The object is generally round in shape.
