This galaxy presents as a relatively luminous object, exhibiting an elliptical morphology with a smooth, featureless profile. It appears nearly circular in projection. The central region displays a slightly brighter and warmer hue, suggesting a concentration of older stellar populations and potentially a weak active galactic nucleus. There are subtle color gradients present across the galaxy, with bluer tones in the outer regions, which may indicate some ongoing star formation. The overall structure shows no prominent spiral arms or bar features, and there are no indications of significant tidal disturbances or recent mergers, although subtle asymmetries or minor disturbances cannot be entirely ruled out given the limited resolution. The galaxy's estimated size suggests it is a substantial system, likely possessing a high stellar mass.
