The galaxy appears as a single, relatively smooth, and concentrated object. It presents an elliptical morphology, appearing mostly round but slightly elongated. It exhibits a diffuse halo, diminishing in intensity outwards from the central core. The core region has a yellowish hue, suggesting an older stellar population or significant dust obscuration. There is no readily apparent spiral structure or evidence of active star formation regions based on the image. The overall impression is that of a quiescent galaxy, possibly an elliptical or lenticular type. There is a slight asymmetry or minor disturbance that may be due to a tidal interaction or a recent minor merger event, but the dominant impression is one of relatively undisturbed, smooth morphology.
