The galaxy presents as an elliptical morphology, with a smooth and centrally concentrated light distribution. The core appears yellowish, possibly indicative of an older stellar population. There is a subtle transition in color towards the outer regions, exhibiting a bluer hue, which may point to the presence of younger stars, even if minimal. The overall shape is somewhat elongated, deviating slightly from perfect circularity. There's no visible evidence of spiral arms, dust lanes, or tidal features suggestive of a recent major merger event; however, a slight irregularity in the outer halo cannot be discounted as evidence of a minor interaction. The galaxy's structure appears mostly undisturbed.
