The galaxy presents as a generally smooth, centrally concentrated structure, likely an elliptical galaxy. It exhibits a high degree of rotational symmetry, with only a slight deviation from a perfectly circular morphology. The light profile appears to decline smoothly from the bright, unresolved core towards the outer regions of the galaxy. There is a subtle color gradient, transitioning from a relatively bluer hue in the central region to a slightly redder color in the outskirts. There is no evidence of strong spiral arms or a well-defined disk structure, nor any significant tidal features suggesting a recent major merger event, although there may be some minor disturbance. The galaxy seems to be relatively isolated and quiescent.
