The galaxy presents as a somewhat elongated, lenticular-like structure. Its central region appears smooth and concentrated, indicating a significant bulge component. The outer regions show hints of a faint, diffuse disk, but the spiral arms are not clearly defined. The color profile suggests an older stellar population, with a yellowish hue dominating. There may be very minor distortions, but the overall morphology appears relatively undisturbed. It may be undergoing transition from spiral to elliptical, or perhaps is a gas-poor spiral that doesn't have active star formation.
