The galaxy presents a largely smooth, elliptical morphology. A concentrated central bulge is evident, displaying a yellowish hue, suggestive of an older stellar population. The outer regions gradually fade in intensity, indicating a decreasing stellar density with increasing radius. There is a slight suggestion of a faint, diffuse disk component surrounding the core region, which may indicate some level of star formation. No prominent spiral arms or significant dust lanes are discernible. Overall, the galaxy appears relatively undisturbed, displaying characteristics of a mature system.
