The galaxy presents an elliptical morphology, exhibiting a smooth, concentrated light profile. The central region displays a yellowish hue, suggesting a population of older stars. Moving outwards from the core, a gradual transition to slightly bluer tones is observed, hinting at the presence of a younger stellar population in the galaxy's outer regions. The overall shape is elongated, with no discernible spiral arms or significant dust lanes visible. There is no indication of major ongoing merger events. The galaxy appears relatively undisturbed, with a smooth and regular structure.
