The galaxy presents as a centrally concentrated object with a relatively smooth morphology. It exhibits a generally elliptical shape, deviating only slightly from perfect circularity. The core region displays a pronounced concentration of light, appearing almost stellar in nature. The color profile suggests a dominant population of older stars, indicated by the redder hue towards the center. The outer regions show a subtle transition to slightly bluer colors, possibly indicating the presence of younger stars and some ongoing, but low, star formation. There is little evidence of distinct spiral arm structures or significant dust lanes. The galaxy appears relatively isolated, without any obvious signs of tidal interactions or ongoing mergers. The overall impression is that of a mature galaxy that is likely in the process of quiescence.
