The galaxy presents a generally smooth, elliptical morphology. Its light profile appears centrally concentrated, with a gradual decrease in intensity towards the outer regions, suggesting an older stellar population. There is a hint of redder coloration in the central region, possibly indicative of dust or a population of older, redder stars. No distinct spiral arms or a prominent disk component are apparent. The overall color suggests a relatively passive galaxy, with low levels of on-going star formation. Faint signs of disturbance are barely perceptible. The object appears round.
