The galaxy appears to be a relatively bright, centrally concentrated object. It exhibits a smooth, elliptical morphology with a dominant spheroidal component and a roughly circular projected shape. The color gradient suggests a population of older stars, giving it a yellowish-orange hue. There are no distinct spiral arms or obvious dust lanes visible. There is faint evidence of a possible tidal tail or plume extending from the main body, indicating a past or ongoing interaction with another galaxy. The object is relatively compact, suggesting it is a massive galaxy. Overall, it presents as an early-type galaxy with signs of potential disturbance.
