The galaxy presents as a barred spiral, with a notable central bar structure spanning a significant portion of the galaxy's apparent width. This bar appears somewhat bright and well-defined, with light distributed evenly across the entire length. The spiral arms extending from the ends of the bar are prominent and somewhat loosely wound. Patches of bright, blue star formation are observed within the arms. The prominence of these blue regions suggests ongoing star formation. The central bulge is moderately sized and indistinct. The disk appears tilted with respect to our line of sight, with the light distribution of the galaxy wider than it is tall. Some asymmetry and disturbances are detected in the outer arms, potentially indicating minor gravitational interactions or tidal effects.
