The galaxy presents as a centrally concentrated elliptical morphology. Its overall color profile indicates a population of older stars, with a yellowish-white central bulge dominating the light output. A faint, diffuse halo surrounds the core, gradually fading into the background. There is very little evidence of spiral arm structure or significant dust lanes; the structure appears largely smooth and homogeneous. Minimal distortion suggests it is not currently undergoing major merger activity. The galaxy appears relatively isolated and undisturbed.
