This galaxy exhibits a complex morphology, possibly indicative of an ongoing or recent interaction with another galaxy. The primary structure consists of a relatively smooth, centrally concentrated component exhibiting a yellowish hue, suggestive of an older stellar population and lower star formation rate. 

A distinct, bluer region is observed adjacent to the main body, offset from the center. The bluer color suggests the presence of younger stars and potentially active star formation. There are also features suggesting some kind of merger or disturbance of the galaxy. The galaxy appears generally oblong in shape.
