The galaxy presents as a centrally concentrated, spheroidal system. There is a dominant, bright core that fades smoothly outward, indicating a high degree of central stellar density. The galaxy exhibits a relatively featureless morphology, lacking any obvious spiral arms or strong dust lane structures. The overall color appears to be yellowish-white, suggesting a population of older stars and a relatively low rate of on-going star formation. There is potentially a hint of blue color in the outer regions of the galaxy. This may suggest the presence of a younger stellar population, but it is difficult to be certain at this resolution. The morphology is consistent with that of an elliptical galaxy. Based on its absolute magnitude, it is likely a large galaxy with a significant stellar mass. There is no indication of a major ongoing merger, although there may be some subtle disturbances in the overall light distribution, indicative of a past interaction.
