The galaxy presents a disturbed morphology, possibly indicative of a recent or ongoing merger event. There's a noticeable disruption in its overall structure, deviating from a simple elliptical or spiral form. Faint tidal features may be present. 

The galaxy exhibits a primarily bluish hue at its center, suggestive of younger stellar populations and ongoing star formation, however, the overall star formation appears low. The galaxy appears to be somewhat concentrated with a diffuse outer halo. The disk appears to be between round and cigar shaped. 