The galaxy appears to be a relatively compact, elliptical-like structure. Its overall color is a pale greenish-blue, with a slight brightening towards the center suggesting a higher concentration of stars in the galactic nucleus. There is a hint of a faint, diffuse halo extending slightly beyond the main body of the galaxy, but no prominent spiral arms or distinct disk features are discernible. The general smooth appearance suggests a lack of ongoing major star formation and an older stellar population. There is no obvious interaction or merging activity readily apparent, although a slight asymmetry cannot be ruled out. The galaxy appears generally undisturbed.
