The galaxy presents as an elliptical morphology, with a smooth, centrally concentrated light profile. The core appears bright and yellowish, suggesting an older stellar population. Moving outwards, the galaxy fades gradually, showing a subtle transition in color to a slightly bluer hue in the outer regions. This color gradient could imply the presence of a younger stellar population at the edges, although it's not immediately apparent in high resolution. The galaxy displays a slight elongation along one axis. There is a hint of a minor disturbance on the right side of the galaxy, it is not immediately clear if the galaxy is involved in an interaction. No distinct spiral arms or significant dust lanes are visible. The overall appearance suggests a massive, relatively evolved system undergoing moderate star formation.
