This galaxy appears to be a spiral type, viewed at an oblique angle. There is evidence of a galactic disc structure, though somewhat disturbed, with a more concentrated bulge region in the center. The central bulge exhibits a relatively smooth, high surface brightness profile, suggesting a significant population of older stars. Faint spiral arms are visible, and some blue coloration is present in the arms, possibly indicating the presence of younger, hotter stars and ongoing star formation. The galaxy does not appear to be perfectly symmetric, displaying some irregularities in the structure of its spiral arms. These distortions suggest possible gravitational interactions or past merger events. There also appears to be a small amount of dust. The dust appears to be obscuring some of the light from the bulge, particularly in the regions closest to the plane of the galaxy, suggesting a concentration in the galaxy's disk. Overall, the galaxy presents as a moderate-mass system, with ongoing though not particularly vigorous star formation and signs of past interactions.
