The galaxy appears as a centrally concentrated, relatively smooth object. Its overall morphology suggests an elliptical type, exhibiting a high degree of rotational symmetry. The light distribution gradually decreases from the center outwards, with no discernible spiral arms or distinct disk-like structures.

The central region exhibits a yellowish hue, potentially indicating a population of older stars. Moving outwards from the center, the colour shifts towards a slightly greener hue. The colour profile suggests a relatively quiescent stellar population with a low rate of ongoing star formation. No signs of major disturbances or tidal features are apparent, hinting at a dynamically relaxed system that is not undergoing or has not recently undergone a major merger event.
