The galaxy presents as a generally smooth and rounded object, with minimal apparent disk-like structures or spiral arms. Its morphology appears elliptical to lenticular. The central region exhibits a bright, concentrated core, suggesting a significant concentration of stars towards the galactic nucleus. The color gradient indicates a redder hue in the central region, possibly indicative of an older stellar population. The outer regions appear slightly bluer, which might imply the presence of some younger stars or ongoing star formation. There is a faint suggestion of a slight disturbance in the overall shape, but no clear signs of a major ongoing merger or significant tidal disruption. The galaxy does not show prominent features such as dust lanes or distinct star-forming regions within the observable image resolution. Overall, the galaxy appears relatively undisturbed and evolved.
