The galaxy presents a largely smooth, elliptical morphology. Its overall shape appears generally round, with only a slight elongation observable. The central region exhibits a high degree of concentration, indicated by the bright, yellowish-white light emission. Moving outward from the core, the luminosity gradually decreases, and the color shifts towards a more bluish hue. The presence of this bluer light likely indicates the presence of a younger stellar population in the outer regions of the galaxy, although their numbers seem low, given the fact that they do not overwhelm the overall older, more yellow stellar population. There is no clear evidence of spiral arm structures or significant dust lanes; however, there is a hint of minor disturbance around the galaxy. This may suggest that this is a recently disturbed system, or that the galaxy experienced a merger event at some point in its past. Overall, this is likely a relatively massive galaxy, and is undergoing a relatively low rate of star formation.
