The galaxy appears as an elliptical or lenticular system, exhibiting a smooth, relatively featureless morphology. The light distribution suggests a centrally concentrated spheroid of stars. There's an indication of some color variation, with a yellower hue towards the center, possibly indicating an older stellar population or dust obscuration. The outer regions are slightly bluer, which could suggest the presence of a younger stellar population, though the effect is subtle. The galaxy is generally round, with no clear evidence of a disk structure or spiral arms. There's no obvious sign of any major merger activity or significant tidal disturbances, although there might be a minor asymmetric feature along one edge. The overall appearance is consistent with a relatively quiescent galaxy, likely with a significant fraction of its star formation having already occurred. The estimated size is a few kiloparsecs.
