The galaxy presents as a relatively smooth, centrally concentrated object. Its overall morphology appears elliptical to lenticular. The light distribution is fairly uniform with a slight color gradient, appearing somewhat redder in the central region and bluer towards the outer edges. There is no distinct spiral arm structure visible in the image. The galaxy shows no major signs of disturbances, such as tidal tails or multiple nuclei, suggesting it has not undergone a major merger event recently. There might be some minor asymmetry or a faint, subtle structure that could indicate a past interaction or accretion event, however, it is not a merger. The moderate blue color in the outskirts implies some level of ongoing star formation, though not at an extreme rate. The lack of prominent dust lanes or patches further supports the relative quiescence of the galaxy. The round shape of the galaxy is very apparent. 
