The galaxy presents as a generally smooth, elliptical-like structure with a concentrated central bulge. There's a gradual decrease in luminosity from the center outwards, suggesting an older stellar population dominates its composition. The galaxy exhibits a yellowish-red hue in the central region, indicative of evolved stars. The overall shape is somewhat elongated, but not extremely so, appearing more "in between" round and cigar shaped, with no obvious spiral arms or disk features visible. There is no apparent major disturbance in the shape or structure. The system appears relatively isolated, lacking prominent tidal features or signs of a recent major merger event, though subtle minor disturbances cannot be ruled out.
