The galaxy presents as an elliptical or lenticular type, exhibiting a generally smooth and rounded morphology. There is little indication of distinct spiral arm structures or significant dust lanes. The light distribution appears relatively uniform across the galaxy's body, although there may be some radial color gradient. The central region appears slightly brighter and more concentrated than the outer regions. The galaxy appears relatively undisturbed, showing no major signs of ongoing mergers or tidal interactions. The galaxy exhibits colors consistent with a population of older stars. 
