The galaxy exhibits a prominent spiral structure with a central bulge. The spiral arms are well-defined and extend outwards from the core, displaying a relatively tight winding pattern. Within the arms, there appears to be evidence of active star formation regions, identifiable as slightly bluer and brighter regions. The central bulge is bright and somewhat concentrated. Overall, the galaxy shows disk features, without appearing to be viewed perfectly edge-on. There is no obvious indication of a major ongoing merger, although some mild asymmetry suggests possible minor interactions or disturbances in the recent past. A faint bar structure appears to be present in the central region. The color distribution suggests an older stellar population dominates in the bulge, while younger stars contribute more significantly to the light emitted from the spiral arms.
