The galaxy appears to be an elliptical galaxy, exhibiting a smooth, centrally concentrated light distribution. It presents a largely featureless morphology, with minimal evidence of spiral arms or distinct substructure. The overall shape is slightly elongated, leaning towards a more oblate spheroidal form. Color gradients suggest a redder core region possibly indicative of an older stellar population and diminishing star formation, surrounded by a bluer, though still subdued, halo. There is no apparent ongoing merger activity or significant tidal disturbances in its immediate vicinity.
