The galaxy presents a generally smooth, elliptical morphology with a slight elongation. A bright, concentrated central bulge is visible, surrounded by a more diffuse halo or disk-like structure. The color profile indicates an aging stellar population, with reddish hues dominating the bulge, suggesting the presence of older, redder stars. Some bluer light is apparent within the outer regions of the galaxy, possibly indicating regions of recent, low level star formation. The galaxy appears relatively undisturbed.
