The galaxy presents as a largely featureless elliptical system. The morphology appears relatively smooth and rounded, with no obvious spiral arm structures or a prominent disk. The central bulge region exhibits a concentrated, bright, golden-yellow hue, suggesting an older stellar population dominated by evolved stars. There is some bluer light present in the outer regions of the galaxy, which suggests ongoing, but perhaps low, star formation, or the presence of a younger population of stars that are moving throughout the galaxy. There is a low probability of interaction with another galaxy or any tidal disturbances. The galaxy's round shape suggests it has either settled down since a collision or has grown through steady, fairly uniform accretion. Overall, the object presents as a mature, fairly massive galaxy undergoing a period of relatively quiescent evolution.
