The galaxy presents an overall ellipsoidal morphology, appearing somewhat elongated. The central region exhibits a higher surface brightness and a yellowish hue, suggestive of an older stellar population likely dominating the core. Moving outwards from the core, there's a transition to a bluer color, especially towards the galaxy's edges. This bluer emission may indicate regions of ongoing or recent star formation. There is some slight evidence of some kind of disturbances on the galaxy, but mostly looks undisturbed.
