The galaxy presents a flattened, elliptical morphology. A prominent, centrally concentrated bulge exhibits a yellowish-white color, suggesting an older stellar population. Fainter, less defined structures extend from the central bulge. The overall structure suggests a possible disk component viewed at a slight inclination. Some asymmetry is apparent in the outer regions, particularly on one side, possibly indicating gravitational interaction or an ongoing merger event. Star formation may be occurring, but is at a relatively low rate.
