The galaxy presents as a relatively smooth, centrally concentrated elliptical type. Its overall shape is generally round, with little to no discernible disk-like features or spiral arms. There may be some minor disturbances in the morphology, but there does not appear to be a major merger or tidal disruption evident. There are no signs of recent major merger activity. The color gradient suggests an older stellar population, with a somewhat redder core. The galaxy appears fairly isolated.
