The galaxy presents as a luminous, elliptical structure. It exhibits a smooth, featureless morphology, lacking prominent spiral arms or a distinct central bar. The light distribution suggests a centrally concentrated luminosity profile, with the brightest region residing in the core. The color gradient transitions from a reddish hue in the center to slightly bluer tinges in the outer regions, indicative of potential variations in stellar populations or dust content across the galactic disk. There appears to be slight disturbance in the galaxy, though not a major one. The overall shape is elongated, though it is not extremely so. There is no obvious sign of tidal tails or merging features, suggesting it is currently not undergoing a major interaction, though minor disturbance suggests it may have undergone one in the past.
