The galaxy appears to be a relatively smooth, elliptical system. It exhibits a bright, concentrated central bulge, with light intensity decreasing gradually towards its outer regions. The galaxy has a generally round morphology, with only slight deviations from perfect circularity. There is no obvious presence of spiral arms or a prominent disk component. The overall color profile suggests a population of older stars, with a yellowish-red hue dominating the light emitted. There are some very slight visual disturbances or asymmetries present in its outer regions but it is largely undisturbed.
