The object presents as a spiral galaxy exhibiting a prominent central bulge, which appears moderately sized relative to the disk. The spiral arms are tightly wound, displaying a high degree of curvature. There appears to be evidence of a bar-like structure extending through the galactic center. Multiple spiral arms can be discerned, with indications of at least four distinct arms. The disk component shows a mottled texture, likely due to regions of star formation. The overall form indicates a relatively undisturbed system, showing no obvious signs of recent major mergers, although subtle disturbances cannot be ruled out.
