The galaxy presents a largely smooth, elliptical morphology. There is an absence of well-defined spiral arms or a prominent disk structure. The galaxy's light is centrally concentrated, with a gradual decrease in surface brightness moving outward from the core. The core exhibits a yellowish hue, possibly indicating an older stellar population, while the outer regions appear slightly redder. The overall shape is generally round, with only a slight deviation towards an elongated form. There may be some minor disturbances or interactions occurring as indicated by some faint asymmetrical features, but no clear merger is in progress. Star formation is low but may still be occurring. The object’s relatively high mass suggest it to be a mature galaxy with a well-developed structure.
