The galaxy presents as a roughly circular object, exhibiting a morphology dominated by a smooth, spheroidal component. The color profile is centrally concentrated, exhibiting a yellowish-orange hue, suggestive of an older stellar population. There appears to be a slight asymmetry or a minor perturbation within the galaxy's structure. The object's overall appearance is that of a relatively undisturbed system, although the possibility of a past minor interaction cannot be ruled out based on the subtle structural deviations.
