The galaxy presents a centrally concentrated morphology, with a smooth and relatively featureless appearance. The core region exhibits a bright, yellowish-white luminosity, suggestive of an older stellar population. Moving outwards from the core, the light intensity diminishes, transitioning into a bluer, less defined halo. There is a slight elongation to the galaxy's overall shape, moving from an almost perfectly circular form towards a more oblate spheroid. No prominent spiral arms or dust lanes are immediately discernible in this imaging. There appears to be some minor asymmetrical structure on the periphery of the disk, potentially caused by minor interactions.
