The galaxy appears as a fairly smooth, elliptical structure with a concentrated central bulge. The color profile suggests a population of older stars, indicated by the reddish-yellow hue of the core. The outer regions display a subtle decrease in surface brightness, with a faint blue tinge suggesting the possibility of some younger stellar populations within the galaxy's disk, though this is not definitively resolved. There is no clear evidence of spiral arms or significant dust lanes. The morphology is relatively undisturbed, without strong indications of recent major merger events or tidal interactions. It presents as a galaxy that is mostly quiescent in terms of star formation.
