The galaxy presents as a luminous, elliptical-type object with a high degree of central concentration. Its overall structure appears smooth, with a lack of discernible spiral arms or distinct features, suggesting it is likely an early-type galaxy. The light profile is centrally bright, fading gradually outwards. The roundness of the object indicates it is closer to an E0 or E1 classification on the Hubble sequence. There is no evidence of ongoing major merging events or significant tidal disturbances.
