The galaxy presents a moderately inclined disk morphology. A prominent, bright central bulge dominates the galaxy's luminosity profile, exhibiting a yellowish-white hue. Fainter, bluer spiral arms extend outwards from the bulge, appearing somewhat diffuse and lacking sharp definition. The disk displays indications of some disturbances, potentially suggesting ongoing or recent minor interactions or mergers. Overall, the galaxy does not present a highly ordered spiral structure, with some asymmetry and irregularities visible in the disk. The galaxy exhibits intermediate star formation activity, based on the bluer color in the spiral arms. The galaxy appears to be an intermediate-mass system.
