The galaxy presents as a relatively compact object with a central, intensely bright core. This core is surrounded by a diffuse halo or disk-like structure that shows a slight elongation. There is evidence of structural disturbance, which might suggest minor tidal interactions or ongoing merger activity with a smaller system. The primary body of the galaxy exhibits bluer colors, particularly in the disk, hinting at younger stellar populations or ongoing star formation. The overall morphology appears to be more disk-like, though with significant deviation from a pure elliptical or spiral form due to the observed disturbances.
