The galaxy presents a generally smooth morphology, with a notable lack of distinct spiral arms or prominent substructure. The light distribution indicates a concentrated central bulge, transitioning to a more diffuse halo. The overall shape is moderately elliptical, tending towards a more spheroidal appearance rather than a flattened disk. The color gradient indicates a relatively uniform stellar population with a dominant older population, concentrated in the center, based on the reddish hue. There are no obvious signs of recent or ongoing major merger events or significant tidal disturbances, although there may be minor internal perturbations. The galaxy exhibits a red-shifted spectrum, indicating a considerable distance. The light profile suggests a fairly quiescent system with a low rate of active star formation, typical of elliptical galaxies.
