The galaxy presents a somewhat disturbed morphology, hinting at potential interactions or internal disruptions. It appears to be a disk galaxy seen at a relatively high inclination. There is evidence of a faint tidal tail or plume extending outwards from the central region, primarily on one side. Within the disk, patchy regions of slightly bluer light are observed, suggestive of localized star formation. The overall color is moderately blue indicating the presence of a young stellar population, though some redder, more evolved stars are still visible towards the center. The estimated size of the galaxy is small and not as luminous, suggesting it may be a dwarf galaxy, or perhaps is farther away than it initially appears. The galaxy exhibits signs of possible minor merging or tidal disturbances, which is likely contributing to the observed star formation and irregular morphology. There are also signs of faint dust lanes within the disk, although they are not very prominent. The overall impression is of a smaller disk galaxy undergoing some form of gravitational interaction or internal activity.
