The galaxy presents as a somewhat diffuse, elliptical form, with a smooth light distribution. The central region appears brighter and more concentrated, suggesting a prominent galactic nucleus. The overall color is slightly redder, indicative of an older stellar population and reduced ongoing star formation. There are no apparent spiral arm structures or significant dust lanes visible. The galaxy does not appear to be strongly interacting with any nearby companions, although there are some faint objects nearby within its vicinity. Its shape is roughly circular, deviating only slightly from perfect symmetry. Based on this, it appears to be a relatively massive and evolved galaxy.
