The galaxy appears to be a relatively smooth, centrally concentrated object. Its overall shape approximates an ellipse, with the major and minor axes being roughly equal. The light distribution suggests a spheroidal morphology, with the intensity peaking sharply at the center and gradually decreasing outwards.

The galaxy exhibits a color gradient, appearing more yellowish-white towards the core, gradually shifting to a slightly bluer hue in the outer regions. There is no evidence of prominent spiral arms or a distinct disk structure. However, subtle color variations and slight irregularities in the light distribution hint at possible faint features within the galaxy. There may be a small chance of a minor disturbance, but the galaxy is mostly isolated.
