The galaxy appears to be a relatively compact object. It exhibits a generally smooth, elliptical morphology with no discernible spiral arm structures or a prominent disk. The central region is brighter and displays a yellowish hue, possibly indicative of an older stellar population. The outer regions of the galaxy fade gradually, showing a slight greenish tint, potentially suggesting the presence of some younger stars or ionized gas, though this feature is not strongly pronounced. There is no apparent tidal disturbance or other signs of a major ongoing merger event. A very slight asymmetry in the outer regions may suggest a minor interaction or disturbance. The overall structure implies a system that is largely relaxed and evolved.
