The galaxy appears as a centrally concentrated, elliptical object. It exhibits a smooth, featureless morphology with a general yellowish hue, suggesting an older stellar population and diminished star formation. The light profile gradually diminishes from a bright core outwards, showing a moderately rounded shape. There are no readily apparent signs of spiral arms, a prominent disk, or ongoing major merger activity. The overall impression is that of a relatively evolved system. There are no major disturbances or merging components visibly interacting with the galaxy.
