The galaxy presents as a centrally concentrated, elliptical-like structure. It displays a smooth, diffuse light profile, lacking any distinct spiral arm features or prominent dust lanes. The core is notably bright and concentrated, suggesting a significant density of stars in the central region. A subtle color gradient is apparent, with the central regions exhibiting a slightly yellowish hue and the outer regions fading to a bluer tint. Overall, the galaxy's morphology appears relatively undisturbed, without any evidence of ongoing major merger events or tidal distortions. There is a suggestion of faint extended halo structure surrounding the main body of the galaxy.
