The galaxy presents a spiral morphology, with prominent spiral arms extending outwards from a central bulge. The arms exhibit a somewhat flocculent structure, with an intermediate degree of winding. The galaxy appears to be relatively face-on.

The central bulge appears significant. There is evidence of a bar-like structure crossing the central region, and a notable population of stars across the galaxy, which suggests moderate star formation activity. Patches of bluer light are visible within the arms, potentially indicating regions of heightened star formation. The overall color suggests an intermediate age stellar population. There is no obvious sign of a strong, ongoing merger event; however, some irregularities in the arm structure could hint at past gravitational interactions. There is no obvious dust lane.
