The galaxy presents a disturbed morphology, suggestive of ongoing or recent interaction. It exhibits a prominent, extended tidal tail extending outwards from the main galactic body, indicating gravitational disruption. The central region appears relatively smooth but with some mottled, diffuse patches. Hints of bluer colors are present within some of these patches. The disk exhibits a relatively irregular shape. A fraction of the community classifies this as a disk that is being viewed edge on, but there is evidence of a galactic bulge which complicates this classification. The galaxy's mass range places it approximately between 10^8 and 10^9 solar masses. The central region has a diameter of approximately 3 kpc. It is exhibiting low star formation rates, as expected given its low redshift. There is a 60% chance that is exhibiting signs of some kind of disturbance, merger, or interaction. The red and green magnitudes are consistent with the overall blueish appearance.
