The galaxy presents as a spiral type, exhibiting a disk-like structure with prominent spiral arms. The arms appear to be well-defined and exhibit a relatively open winding pattern. Two distinct arms are readily discernible. The central bulge is relatively small and not particularly luminous compared to the disk. There is evidence of a bar-like structure traversing the central region, potentially a weak bar given its morphology. The galaxy shows no obvious signs of major mergers or significant tidal disturbances, but there is a subtle asymmetry suggesting a possible minor interaction. Patches of active star formation are hinted at within the spiral arms, evidenced by variations in color and luminosity.
