This galaxy presents as a moderately bright, elliptical-like structure. It exhibits a generally smooth light distribution, with a subtle color gradient towards the core. The galaxy has a slightly diffuse appearance, with no clearly defined spiral arms or bar features. A marginal asymmetry suggests a potential minor interaction or disturbance, though the overall morphology appears relatively undisturbed. There may be minor dust lane features as well, although it may be an artifact. The object's color suggests a population of older stars, potentially indicating a relatively low current star formation rate. The compact appearance implies it could be a galaxy with a fairly high stellar mass.
