The galaxy presents as a smooth, elongated structure, suggestive of an elliptical morphology. Its color profile indicates a central, concentrated region exhibiting a yellowish hue, possibly indicating an older stellar population. The outer regions display a bluer tint, which may signify the presence of younger stars or regions of ongoing star formation. Overall, the galaxy appears relatively undisturbed, with no signs of major mergers or significant tidal disruptions. There is a subtle asymmetry to the outer regions, which could be the result of a minor disturbance.
