The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. The core region exhibits a yellowish-white hue, suggesting an older stellar population. Moving outward from the center, the color shifts to a more bluish tint, possibly indicating the presence of younger, hotter stars. The morphology is primarily smooth, with little evidence of prominent spiral arms or significant dust lanes. There is a slight asymmetry, with the light extending more along one axis. No major disturbances or signs of ongoing merging are readily apparent. The general appearance suggests an evolved system. The overall color profile indicates a moderate level of recent or ongoing star formation activity.
