The galaxy appears as a single, largely featureless object with a smooth light distribution. Its morphology suggests a classification leaning towards elliptical or lenticular. The overall color is somewhat red, potentially indicating an older stellar population with suppressed recent star formation. There might be a faint disk component, but the resolution is not sufficient to confirm. There is a suggestion of minor disturbances to the morphology, but no major merger events are observed. The galaxy seems to be an isolated system with no nearby companions significantly impacting its structure.
