The galaxy presents a generally smooth, elliptical morphology. There is a central concentration of luminosity which may indicate a dense stellar population, potentially an active galactic nucleus. The overall color profile suggests a higher proportion of older stars, exhibiting a yellow to reddish hue. There is a marginal indication of a disk, but not a significant or distinct feature. There may be some signs of disturbance, but no major merger is occurring. The overall appearance is of a relatively undisturbed, evolved system.
