The galaxy presents as a moderately small, disk-like structure. The central region exhibits a brighter, more condensed area, possibly indicative of a galactic bulge. The disk shows some subtle features, including hints of spiral arm structures or irregular dust lanes. These features are not sharply defined, suggesting either a more flocculent spiral design or a degree of disruption. Color variations across the galaxy are subtle, with a slightly bluer tint in certain regions, potentially indicating areas of recent star formation. The overall morphology suggests a galaxy undergoing some level of interaction or disturbance, though not in a dramatically advanced stage of merging.
