The galaxy presents as a centrally concentrated object with a moderately smooth overall appearance. It exhibits a dominant spheroidal component with a relatively high degree of roundness, showing a subtle elongation. The central region is notably brighter than the surrounding areas. There is evidence of some faint disk-like feature extending outward with slight asymmetries in the outer regions. Some indications of minor disturbances or interactions, but overall does not have distinct merging features. The galaxy has a reddish hue, likely due to dust obscuration or the presence of older stellar populations.
