The galaxy presents as a moderately luminous, elliptical-like structure with a smooth and diffuse appearance. It exhibits a noticeable central bulge that is more concentrated and brighter than the surrounding halo. The colour gradient suggests a slightly redder core, possibly indicating an older stellar population centrally located. There is little evidence of distinct spiral arms or significant dust lanes. The galaxy appears relatively isolated, lacking any obvious signs of tidal interactions or major mergers, although there may be some minor disturbances to its morphology. The overall impression is of a galaxy that is either in the process of, or has recently completed, a transition to a more quiescent state, with a modest rate of star formation.
