The galaxy presents as a single, somewhat symmetrical structure dominated by a smooth, centrally concentrated component. It appears largely elliptical in overall shape. The galaxy exhibits a color gradient, with a yellowish-green hue at its core gradually transitioning to a more reddish outer region. This suggests a possible gradient in stellar populations, with relatively younger, hotter stars concentrated in the central region and older, cooler stars dominating the outer parts. There appears to be little evidence of spiral arm structure, active star formation regions, or dust lanes within the main body of the galaxy. The overall visual impression is that of a relatively evolved system, perhaps with a diminishing star formation rate. There appears to be a small nearby object which could be interacting.
