The galaxy presents as a spiral galaxy, observed at a significant inclination to our line of sight. The presence of spiral arms is indicated, with a moderate degree of winding. The galactic bulge appears relatively small compared to the overall galactic disk. No strong bar structure is immediately obvious in the central region; however, some elongated feature exists. The disk exhibits a notable degree of patchiness, suggesting ongoing star formation regions. The overall morphology indicates the galaxy has not undergone a recent major merger event, although potential minor disturbances are visible in the outer regions of the disk. Colors range from blue to red, with blue concentrated in the disk areas, indicating younger stars and ongoing star formation. Red color dominates the core area. The estimated size of the galaxy's half-light radius is around 7 kpc.