The galaxy presents as a generally smooth, elliptical morphology. The light profile appears centrally concentrated with a gradual decrease in surface brightness away from the core. The core region exhibits a yellowish-white hue, suggestive of an older stellar population. Fainter, bluer regions are sparsely distributed throughout the galaxy, indicating some potential for ongoing, albeit low, levels of star formation. There is no clear evidence of a spiral structure, bar, or significant tidal disturbances. The galaxy appears relatively isolated and undisturbed. The axial ratio suggests a moderate degree of ellipticity, being somewhere in between round and cigar shaped. 
