The galaxy presents as a face-on spiral, exhibiting a distinct disk structure with prominent spiral arms. The arms are loosely wound and extend from a central bulge. The bulge itself appears moderate in size and luminosity. Traces of a possible stellar bar are faintly visible across the central region.

Blue hues are prominent throughout the disk, suggesting active star formation. Patches of increased luminosity are present within the arms, indicative of star-forming regions or young stellar clusters.

There appear to be signs of gravitational interaction, with some asymmetry and disturbance in the outer regions of the disk and spiral arms. It is difficult to determine if this is a minor disturbance or a full fledged merger with another galaxy.
