The galaxy presents as a diffuse, relatively smooth elliptical galaxy. It exhibits a moderate central concentration of light, fading gradually towards its outer edges. The color profile indicates a fairly uniform population of older stars, with a slight reddening towards the core suggesting a possible accumulation of dust or a higher concentration of older, redder stars. There's little evidence of spiral arm structure or prominent dust lanes. The overall shape appears nearly circular, showing no major distortions indicative of recent merger activity although there are some minor disturbances. The galaxy displays low star formation. 
