The galaxy presents a somewhat disturbed morphology, exhibiting characteristics intermediate between a smooth elliptical and a disk galaxy. It appears elongated, more "in between" rounded and cigar-shaped than either perfectly circular or extremely elongated. The galaxy shows a bright, concentrated central bulge that is roughly spherical and yellowish in color, indicative of an older stellar population. Fainter, more diffuse material surrounds the bulge, suggesting a disk-like structure or envelope. There appear to be signs of tidal disturbances or ongoing interactions, with some asymmetry and faint extensions visible in the outer regions. These distortions imply recent or ongoing merger activity. There appears to be moderate levels of star formation. The disk component is relatively faint and not sharply defined.
