The galaxy appears to be an elliptical galaxy, exhibiting a smooth, concentrated light profile with minimal discernible features. It presents as a relatively homogenous structure with a slight elongation, not perfectly spherical. There is no visible spiral arm structure or dust lane obscuration. The galaxy's color suggests a population of older stars, indicating relatively low current star formation activity. The morphology is consistent with a galaxy undergoing little to no merging activity or major disturbance. The central region of the galaxy appears brighter than its outer regions, indicating a possible concentration of stars towards the core.
