The galaxy presents a largely smooth morphology, appearing elliptical in shape. It exhibits a concentrated central bulge that emits strongly in yellow light. The outer regions display a fainter, more diffuse halo with a slight flattening along the equatorial plane, and hints of bluer light. There is no clear evidence of spiral arm structure, significant dust lanes, or ongoing major merger activity. The galaxy seems to be relatively isolated and well-defined, with only minor disturbances possibly present.
