The galaxy presents as a centrally concentrated elliptical or lenticular system. It exhibits a smooth, featureless morphology with a high degree of rotational symmetry. The color profile suggests an older stellar population, with a redder hue. There is no apparent disk structure or spiral arm features visible. The system appears relatively isolated, without significant tidal disturbances or nearby companions indicating recent or ongoing mergers. There are two other similar appearing galaxies nearby, but it is unclear if these galaxies are gravitationally interacting with the primary one.
