The observed galaxy presents a primarily smooth morphology, exhibiting a bright, concentrated central bulge. There is a hint of a possible disk component, suggested by the slight flattening and extension along a preferred axis. The dominant color is bluish-white, particularly in the core, which may suggest the presence of hotter, younger stars or active galactic nuclei activity. Faint tidal features or disturbances are subtle but can be seen as irregular edges on the galaxy; it is possible that they are the result of minor interactions. The overall structure is somewhat compact, with a relatively small angular size.
