The galaxy presents as a relatively smooth, centrally concentrated object. Its overall shape appears elliptical, with a high degree of roundness. There is no obvious disk structure or spiral arm morphology visible. A subtle color gradient is present, with the central region exhibiting a yellowish-white hue indicative of an older stellar population. The outer regions transition to a slightly bluer color, possibly suggesting more recent, albeit subdued, star formation. There is no evidence of major mergers or significant tidal disturbances impacting the galaxy's morphology. The estimated size is on the order of several kiloparsecs in radius.
