The galaxy exhibits a primarily smooth morphology with a dominant spheroidal component. The central region is characterized by a high concentration of light, appearing nearly circular in shape. The color profile indicates a generally older stellar population, presenting a yellowish-orange hue that suggests a lack of significant ongoing star formation. There is a faint, diffuse halo surrounding the central bulge. The overall structure appears relatively undisturbed, with no apparent signs of major mergers or tidal interactions. Weak evidence of a disk like structure is visible but not dominant.
