The galaxy presents a predominantly smooth, elliptical morphology. There is little evidence of spiral arm structure or significant dust lanes. The central bulge appears bright and relatively concentrated, exhibiting a yellowish-orange hue indicative of an older stellar population. The galaxy displays a slight elongation, deviating minimally from a perfectly circular form. There are subtle color gradients observed moving from the core to the outer regions with an intensity of blue. There does not appear to be evidence of any ongoing major mergers or significant tidal disturbances affecting the galaxy's overall structure. The galaxy's overall appearance is consistent with that of a well-evolved, relatively quiescent system.
