The galaxy presents an elliptical morphology, with a centrally concentrated bulge that gradually fades into an extended halo. The color profile suggests an older stellar population, with a reddish hue dominating the central region. The outer halo exhibits a bluer tint, hinting at the presence of younger, star-forming regions, or a recent minor merger that introduced a new population of stars. A faint, elongated structure extends from the central bulge, potentially indicating a tidal tail or disturbance caused by a past gravitational interaction. The overall appearance indicates a likely intermediate-mass system undergoing a transition from a more actively star-forming phase to a quiescent, redder state.
