The galaxy presents a generally elliptical morphology, exhibiting a smooth, relatively featureless structure. Its color profile is notably redder in the central region, suggesting a higher concentration of older stellar populations. The outer regions display a slightly bluer hue, which might indicate the presence of younger stars, albeit at a lower density compared to the galactic nucleus. The overall shape appears elongated, deviating slightly from a perfect sphere, and lacks any clear signs of spiral arms or significant dust lanes. There may be very slight disturbances, but is generally smooth. There appears to be a concentration of mass towards the center of this galaxy. 
