The galaxy presents a generally smooth, elliptical morphology with a centrally concentrated luminosity profile. The core exhibits a yellowish-white hue, indicating a population of older, evolved stars. A subtle radial color gradient is visible, transitioning to a slightly redder hue in the outer regions, potentially indicating a decline in recent star formation activity with increasing distance from the galactic center. There is little indication of spiral arm structure or significant dust lanes. Minor disturbances can't be ruled out, however it has a generally settled structure, with no obvious tidal features or ongoing major mergers evident in the image. The galaxy appears approximately round.
