The galaxy appears to be a relatively smooth, elliptical galaxy. It exhibits a concentrated central bulge that transitions gradually outward into a more diffuse halo. The core of the galaxy presents a yellowish hue, possibly indicating a population of older, cooler stars. The outer regions display a bluer tint, suggesting the presence of some younger, hotter stars, although their numbers appear to be small. The galaxy has a slightly elongated shape, deviating moderately from perfect circularity. There is no immediately apparent evidence of spiral arms, dust lanes, or a recent major merger event. Minor disturbances or interactions cannot be ruled out. The object is of intermediate size.
