The galaxy presents as a disk galaxy, observed at a significant inclination to our line of sight. There is evidence of a central bulge component. The disk exhibits a mottled texture with indications of spiral arm structure, though poorly defined, suggesting a flocculent or disrupted morphology. Patches of bluer color are scattered throughout the disk, possibly indicating regions of active star formation. The isophotes of the galaxy appear elliptical. The galaxy appears relatively smooth and somewhat more concentrated towards the center. There seems to be a second dwarf galaxy nearby, though it is much smaller and less distinct than the main galaxy.
