The galaxy appears as a centrally concentrated object with a relatively smooth, elliptical morphology. The core exhibits high luminosity, gradually fading into a more diffuse outer region. There is a subtle blue tint to the central region that fades out farther from the core. Evidence of some irregularities are present in the outer regions, which appear as minor disturbances that could indicate a recent interaction or merger event. There is no clear disk structure visible; it is not possible to determine if it is a spiral. The overall impression is that of a galaxy undergoing either a quiet evolution or a period of post-merger relaxation.
