The galaxy presents as a relatively smooth, elliptical-like structure. The central region exhibits high luminosity, appearing as a bright, concentrated core. Moving outwards from the core, the luminosity gradually decreases, forming a diffuse halo or envelope. There is little to no discernable spiral arm structure or dust lane features. The overall color appears bluish, potentially indicating the presence of a younger stellar population within the galaxy, though this may also be influenced by redshift. A subtle asymmetry in the outer regions might suggest a minor interaction or disturbance, but the overall morphology favors a relatively relaxed, non-merging system. The galaxy appears somewhat flattened.
