The galaxy exhibits a disturbed morphology, appearing to be undergoing a merger or interaction. Its shape is irregular and shows evidence of tidal features or disrupted arms. The central region displays a yellowish hue, suggestive of an older stellar population, while more diffuse and elongated regions exhibit a greenish tint. The green regions may indicate the presence of ongoing star formation. The overall luminosity of the galaxy suggests it is a relatively massive system. The galaxy appears to be the result of the merger of multiple systems, as suggested by the irregular shape, and tidal features.
