The galaxy presents as a moderately luminous, elliptical-shaped structure, exhibiting a smooth, featureless morphology. A concentrated central bulge is evident, displaying a yellowish hue indicative of an older stellar population. The outer regions of the galaxy appear more diffuse, with a subtle transition towards bluer colors, suggesting the possibility of some ongoing, albeit limited, star formation within the galaxy's extended halo. There are no readily discernible spiral arms or bar structures. Minor disturbances may be present, but the overall structure is largely undisturbed. The galaxy appears relatively isolated, showing no clear signs of a major merger event.
