The galaxy presents as a slightly distorted, disk-like structure with a bluish hue. It exhibits moderate internal texture and is centrally concentrated, with a bright core that diminishes outwards. Evidence of ongoing or recent merging activity is apparent, with possible tidal features or distortions present in the outer regions. The spiral arm structures, if present, are not well-defined. This object is likely a late-type spiral galaxy, but the degree of disturbance suggests interactions may be influencing its morphology. The overall color indicates ongoing star formation, though it appears moderate.
