The galaxy appears to be a relatively compact object, exhibiting a smooth, elliptical morphology. A concentrated, bright central region is visible, suggesting the presence of a galactic bulge. The light profile decreases gradually from the core outwards, fading into the surrounding background sky. The galaxy appears yellowish, indicating a population of older stars. There is no sign of spiral arm structure or significant dust lanes. The overall impression is that of a quiescent system, likely with a low star formation rate.
