The galaxy presents as a face-on or nearly face-on spiral galaxy with a prominent central bulge. The bulge exhibits a smooth, yellowish-white hue, suggesting an older stellar population. A faint, diffuse disk surrounds the bulge, showing some evidence of spiral arm structure, though not sharply defined. These arms exhibit a slightly bluer tint than the bulge, implying the presence of younger, hotter stars. The overall shape of the galaxy is moderately elliptical. There is some hint of a bar-like structure extending across the central region. The galaxy appears relatively isolated, with no immediate signs of major interaction or tidal disruption.
