The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. It exhibits a yellow-white hue, indicative of a population of older stars. No distinct spiral arms or dust lanes are apparent. The galaxy appears nearly circular in shape. There is no clear evidence of tidal tails or significant morphological disturbances suggesting a recent major merger event, but there may be some subtle unevenness in the outer regions of the galaxy. Overall, the galaxy appears relatively isolated and quiescent.
