The galaxy presents as a relatively smooth, centrally concentrated structure. It exhibits a flattened, disk-like morphology, although the inclination angle obscures a clear view of spiral arm features. A bright, prominent bulge dominates the central region, appearing approximately round. The color gradient suggests a population shift, with the central bulge exhibiting a yellowish-white hue, indicative of older stellar populations, while the outer disk shows bluer tones, hinting at ongoing star formation. There is a subtle indication of a disturbance or asymmetrical feature in the outer regions of the disk. The galaxy is approximately 9.5 kpc across, suggesting it is a medium sized galaxy.
