The galaxy presents a distinct spiral structure. The spiral arms are prominent, with a moderately wound morphology extending outwards from a central bulge. The bulge exhibits a moderate size relative to the overall disk.

There is a suggestion of two major spiral arms. The disk is viewed at an angle far from edge-on. The galaxy appears to be relatively isolated with no immediately apparent major merging or tidal disruption.

There is evidence of active star formation within the spiral arms, with visible star-forming regions. No strong bar-like structure is discernible.