The galaxy presents as a centrally concentrated object with a generally smooth appearance. Its light is dominated by a bluish-green hue, suggesting a notable population of hot, young stars and ongoing star formation, although it appears to contain older stars as well. The light distribution appears largely elliptical with a round shape, and a smooth profile, with what appears to be a lack of spiral arms. The overall structure hints at a potential quiescent state or a recent interaction that has disrupted prior structures. There is no clear evidence of strong tidal features or a major ongoing merger from what I can see. There is faint light suggesting very weak outer edges. 
