The galaxy appears as a singular, concentrated luminous object with a generally smooth morphology. It exhibits an elliptical-like structure with no readily apparent spiral arm features. The overall color of the galaxy is yellowish-orange suggesting a population of older stars dominating its stellar content. There are some localized, slightly bluer areas near the center of the galaxy, hinting at a presence of younger, hotter stars and possibly ongoing or recent star formation, albeit at a relatively low rate. The galaxy appears relatively undisturbed, lacking any obvious signs of a major ongoing merger or tidal disruption. There is no evidence of a prominent, extended disk structure, which is consistent with an early-type galaxy classification. Its roundness indicates it is more likely a near face-on system.
