The galaxy presents as a largely smooth, elliptical or lenticular structure. It exhibits a concentration of light toward its center, indicative of a prominent bulge. There is a slight elongation, deviating from a perfectly circular shape. The galaxy's color profile suggests an older stellar population, with a dominant yellowish-orange hue, this could point to lower levels of recent star formation. Subtle irregularities in the outer regions may hint at minor disturbances or interactions, but these are not particularly prominent. The overall structure appears relatively undisturbed, indicating an evolved system, likely with minimal ongoing merger activity.
