The galaxy presents a smooth, elongated morphology, indicative of an elliptical galaxy. Its color profile exhibits a subtle gradient, transitioning from a slightly bluer hue towards the outer edges to a more reddish-yellow core. This color distribution might suggest the presence of a relatively older stellar population concentrated within the central region, with younger, bluer stars distributed in the outer parts. The galaxy displays minimal signs of spiral arm structures or significant dust lanes, further supporting its classification as an elliptical galaxy. There is no clear evidence of any ongoing major merger events or significant tidal distortions. A slight asymmetry in the outer isophotes might suggest a past minor interaction, but the overall structure appears relatively relaxed and undisturbed.
