The galaxy presents an overall smooth morphology, appearing generally elliptical when considering its shape. The light distribution suggests a central bulge, with a concentration of older stars, indicated by the yellowish hue. Fainter, bluer regions surround the bulge. There is a hint of disk-like structure, though it does not have clearly defined spiral arms. The object is not perfectly circular. The galaxy exhibits no signs of a recent or ongoing major merger event. Minor irregularities are apparent at the periphery, suggesting possible minor interaction or tidal effects. The galaxy is relatively compact.
