The galaxy presents as an elliptical or lenticular type, with a generally smooth, featureless appearance. It exhibits a high degree of central concentration, with a bright, compact core that gradually diffuses outwards. The galaxy appears round and generally undisturbed. There may be faint hints of a disk-like structure surrounding the core, however the lack of readily observable spiral arms or dust lanes suggests that its disk is not dominant. The galaxy exhibits a redder hue near the core, transitioning to bluer tones in its outer regions. This color gradient likely indicates a central population of older stars with younger stars populating the galactic outskirts. Star formation appears low.
