The galaxy presents a complex morphology, exhibiting characteristics suggesting an ongoing or recent merger event. A dominant, relatively smooth, and centrally concentrated component displays a yellowish hue, potentially indicative of an older stellar population. This component is juxtaposed with a bluer, less defined region, possibly associated with active star formation triggered by the interaction. Evidence of tidal features or extended structures is subtle, but there are hints of minor disturbances in the overall structure. The shape is somewhat irregular, leaning towards an elongated or in-between profile rather than a perfect circular symmetry. Overall, the galaxy appears to be a moderately luminous object with a mass consistent with a typical spiral or small elliptical galaxy, experiencing a significant interaction event influencing its star formation rate and morphology.
