The galaxy presents as a spiral galaxy. The disk is prominent and oriented approximately face-on relative to our line of sight. Two discernible spiral arms exhibit a moderate winding pattern, with a relatively high degree of symmetry. No central bulge is visible, and a bar structure seems to be present within the central region.

Based on visual morphology, the galaxy displays signs of a possible interaction or merging event, as evidenced by distortions in the overall structure. Specifically, there is a prominent tidal tail. This suggests the recent or ongoing tidal interaction.

The overall color profile indicates active star formation, based on the blue hues, particularly within the spiral arms.
