The galaxy presents a largely smooth, centrally concentrated morphology. There is a discernible radial gradient in color, transitioning from a yellow-white hue in the core to a bluer halo. The object appears moderately luminous and relatively compact with only a mild indication of asymmetry or disruption to the main body. There may be a minor disturbance visible at the bottom of the galaxy. Given the smooth appearance and color profile, the galaxy is potentially an elliptical or an early-type spiral. The observed colors indicate the presence of intermediate-age to old stellar populations. A moderate level of star formation is likely occurring.
