The galaxy appears as a relatively smooth, elliptical structure, exhibiting a concentrated central bulge. The morphology suggests it is likely an early-type galaxy. A slight elongation is apparent, trending towards a flattened, though not disklike, shape. The light profile appears centrally concentrated. There is little evidence of prominent spiral arms or significant dust lanes. There may be some minor disturbances present in the overall structure, suggesting a possible interaction or minor merger history. The color gradient suggests a generally older stellar population throughout the galaxy.
