The galaxy presents as an elliptical morphology, elongated along a distinct axis. Its core region exhibits a concentrated, bright yellow-gold color, suggesting a population of older stars. Proceeding outward from the core, the light gradually diminishes and becomes redder, particularly at the polar ends of the major axis, indicating either dust obscuration or older stellar populations in these regions. The overall smooth appearance suggests a relatively evolved system. The structure appears undisturbed and unperturbed. There is no evidence of spiral arms or a disk-like structure.
