The galaxy appears to be a relatively luminous and massive system, exhibiting a predominantly smooth morphology. The light is concentrated towards the center, indicative of a well-defined bulge or core. There is a slight color gradient from the core, which shifts from yellow to green. Faint disturbances are present in the form of subtle asymmetries or possibly tidal features, suggesting past interactions or internal dynamical processes. There is the presence of some recent or ongoing star formation. The galaxy does not show any signs of a prominent disk structure or spiral arms, consistent with an early-type galaxy classification. The round shape suggests it could be an elliptical galaxy.
