The galaxy presents as a relatively smooth, elliptical-like structure with a dominant central bulge. The color profile suggests an older stellar population, appearing primarily yellow-orange. There is a subtle gradient in color, transitioning from a brighter, more yellow core to a redder, more diffuse outer region. No distinct spiral arms or dust lanes are readily apparent. Overall, the morphology indicates a galaxy that is not actively undergoing major star formation events and is in a relatively quiescent state. There are no obvious signs of tidal interactions or major disturbances in the galaxy's structure, such as pronounced asymmetries or extended tidal tails.
