The galaxy appears to be a spiral galaxy, exhibiting a discernible disk structure. The spiral arms are not tightly wound but rather open and somewhat flocculent. Patches of bluer light are visible along the spiral arms, suggesting regions of active star formation. The central bulge is moderately sized. The galaxy presents no obvious signs of a major ongoing merger, though there may be some minor disturbances or faint tidal features implying past interactions. The overall color index indicates a mix of stellar populations, with a relatively old stellar population dominating the bulge and younger stars populating the spiral arms. The galaxy is viewed at an angle oblique to its plane, and the bar appears to be weak or nonexistent.
