The galaxy presents as a diffuse, elliptical morphology with a smooth light distribution. The central region exhibits a bright, concentrated core, suggesting a high stellar density. Moving outward from the core, the light intensity gradually diminishes, with a relatively smooth transition to the outer regions. The galaxy displays a slight elongation along its major axis. The color gradient appears subtle, with the central regions exhibiting a yellowish-orange hue, potentially indicating an older stellar population. The outer regions appear slightly bluer, possibly indicating the presence of younger stars or ongoing star formation. There is no obvious evidence of spiral arms, prominent dust lanes, or significant tidal disturbances. The overall appearance suggests a relatively evolved galaxy, potentially an elliptical galaxy, undergoing low levels of star formation.
