The galaxy presents a complex morphology, suggestive of an ongoing or recent interaction. A prominent feature is a brighter, somewhat spherical component, exhibiting a bluish hue. This may indicate a region of active star formation. Connected to this component, a more elongated structure extends outwards, displaying a gradient of colors from a central yellowish-red to a fainter blue at the periphery. The overall impression is of a system undergoing some level of disturbance, possibly involving a merger or tidal interaction between galactic components. The features hint at both a smoother, more established stellar population and regions of more recent starbirth. There appears to be a tidal tail. The size of the galaxy is rather large, and the amount of star formation is modest.
