The galaxy presents as a spiral type with a clearly defined, albeit somewhat amorphous, disk structure. Two spiral arms are prominently visible, exhibiting a moderately loose winding pattern. The central bulge region appears relatively small, and possesses a yellow/white color implying an older stellar population. The disk component displays a mottled blue hue, indicative of ongoing star formation. There are disturbances apparent in the disk, suggesting that there may be some merging or tidal interaction occurring.
