The galaxy presents as a smooth, elliptical-like structure. Its morphology is predominantly smooth, with a noticeable lack of spiral arms or distinct disk features. The light distribution appears centrally concentrated, with a bright core that gradually fades towards the outer edges of the galaxy. The overall shape is elongated, deviating from a perfectly circular form, with the major axis extending more than the minor axis. There is no apparent sign of any major merger events or significant tidal disturbances. Close inspection hints at some minor disturbances within the outer halo. Color analysis suggests a higher concentration of older stars, as indicated by the yellowish hue.
