The galaxy presents as a luminous, elliptical system with a smooth morphology. Its color appears primarily yellow-orange, suggesting an older stellar population with relatively low ongoing star formation. The galaxy exhibits a centrally concentrated light profile, with a gradual decrease in brightness outwards from the core. There is no apparent structure such as spiral arms or a prominent disk. The overall round appearance suggests it is unlikely to be a highly inclined spiral galaxy. The system does not obviously appear to be undergoing any major merging events or significant tidal disturbances, suggesting it is relatively settled. The galaxy is a substantial system, implying it is relatively massive.
