The galaxy presents as an elliptical morphology, exhibiting a smooth and concentrated light profile. The color gradient is subtle, transitioning from a more yellowish central region to slightly redder outskirts. There are no discernible spiral arms or significant dust lanes visible in this observation. The overall appearance suggests a relatively evolved system, likely with a dominant population of older stars and a low rate of current star formation. There are no obvious signs of tidal disturbances or ongoing major mergers. The shape is somewhere between round and elliptical.
