The galaxy appears to be a relatively small, low-mass system. Morphologically, it presents a somewhat irregular shape, possibly indicative of tidal interactions or internal disturbances. The galaxy exhibits a subtle color gradient, with a bluer region concentrated on one side. This bluer area suggests ongoing or recent star formation. The overall structure lacks a well-defined spiral arm structure or prominent bulge, indicating a less-organized or disrupted morphology. The galaxy's light is moderately faint, suggesting a low luminosity.
