The galaxy presents as an elliptical structure, elongated along its major axis. Its morphology appears smooth, lacking readily discernible spiral arms or distinct features. The color gradient indicates a possible concentration of older stellar populations towards the center, which exhibits a yellowish hue, transitioning to bluer tones in the outer regions. There is a suggestion of minor disturbances or interactions within the galaxy, potentially indicating past merger events or tidal interactions, though the overall form remains largely undisturbed. The galaxy's estimated size is relatively modest, but its absolute magnitude suggests that it is luminous. The galaxy's star formation rate is low, which supports its classification as an elliptical galaxy composed primarily of old stars.
