The galaxy presents a generally elliptical morphology, appearing nearly circular in projection. It exhibits a smooth, centrally concentrated light distribution, characteristic of an early-type galaxy. A bright, yellowish core is observed, indicative of an older stellar population. The outer regions show a gradual decrease in luminosity with a subtly bluer hue, hinting at a minor population of younger, bluer stars. There is no discernable spiral structure or active star formation regions visible in this observation. The overall appearance suggests a relatively quiescent galaxy with a minor amount of ongoing star formation, possibly due to a recent minor merger or accretion event.
