The galaxy presents a somewhat elliptical morphology. It displays a smooth light distribution, appearing mostly featureless upon visual inspection, with some indication of a diffuse disk component. The central region exhibits a concentrated brightness, suggesting a prominent galactic nucleus. The color gradient indicates a redder core, transitioning to bluer hues in the outer regions, potentially reflective of varying stellar populations and star formation activity. There are suggestions of minor asymmetry or disturbance in the halo, possibly stemming from an ongoing or past interaction. The estimated size indicates this is a fairly sizable galaxy. Overall, it seems to be a relatively evolved galaxy.
