The galaxy presents as a somewhat smooth, elliptical-like structure with a concentrated central bulge that appears brighter and more luminous than the surrounding regions. The galaxy exhibits a dominant, round morphology with a slight deviation toward an intermediate ellipticity. No prominent spiral arms or distinct disk features are discernible in the available imagery.

There may be evidence of minor disturbances in the outer regions, though the overall structure appears relatively undisturbed, and the galaxy shows no signs of major mergers or significant tidal interactions. The stellar population appears generally old, with limited ongoing star formation inferred from the color distribution.
