The galaxy presents a largely smooth, elliptical morphology. There is an absence of clearly defined spiral arms or a prominent disk structure. Its shape is generally round. The light distribution appears relatively even, with no significant central bulge dominating the overall brightness. There is a subtle color gradient, with a slightly redder hue towards the core region and a bluer hue towards the edge. This suggests an older stellar population dominates this galaxy. There are no obvious signs of ongoing major merger activity.