The galaxy appears to be a spiral galaxy, exhibiting a clear disk structure with prominent spiral arms. The arms show a mixture of medium and loosely wound morphologies, traced by regions of enhanced luminosity suggesting areas of active star formation. The color variations within the arms indicate varying stellar populations.

The bulge component appears moderate in size, and the presence of a bar feature is subtle but possible.

The galaxy exhibits evidence of potential gravitational interaction or recent merger activity, characterized by disturbances in the spiral arm structure and overall morphology. These disruptions suggest possible tidal interactions with a nearby companion galaxy.
