The galaxy appears to be a single, relatively smooth, centrally concentrated object with a distinct elliptical morphology. The light profile suggests a high degree of radial symmetry. The core exhibits a bright, yellowish hue which fades outwards with decreasing surface brightness. There is no discernible spiral structure, bar, or tidal features apparent in the image. The galaxy's color and lack of features indicate an older stellar population dominated by evolved stars, and a high likelihood of being an early-type galaxy. The galaxy's overall roundness suggests it is likely an E0-E2 elliptical galaxy. There appears to be minimal dust extinction and low ongoing star formation. No evidence of a recent or ongoing merger event is observed.
