The galaxy presents a predominantly smooth, elliptical morphology. It appears significantly rounded, with only a subtle elongation. There is no strong evidence of spiral arm structure or prominent dust lanes. The central bulge is bright and dominant, gradually fading into a less luminous halo. There appears to be no significant evidence of recent or ongoing major merger events. The faint outer regions suggest a quiescent environment with minimal star formation activity, although the bluer color of the inner disk hints at some continuing level of younger stars. 
