The galaxy appears to be an elliptical, with a smooth, centrally concentrated light profile. It exhibits a fairly uniform yellowish-white color, which is likely indicative of an older stellar population with a low rate of ongoing star formation. The galaxy's shape appears somewhat rounded. There is no visual evidence of spiral arms, a disk, or significant dust lanes. There does not appear to be evidence of any recent major merger events that may be visibly distorting the morphology. Overall, the galaxy presents a morphology consistent with a passively evolving system.
