The galaxy presents as a centrally concentrated object, exhibiting a generally smooth, elliptical morphology. It displays a subtle color gradient, transitioning from a slightly reddish core to a bluer outer halo. This may indicate an older stellar population concentrated towards the galaxy's center and younger star formation in the outer regions. No distinct spiral arm structures or a prominent disk are discernible. There is no strong indication of any ongoing major merger events, although some minor asymmetry may be present in the outer reaches. The overall roundness of the galactic shape is apparent, with a mild ellipticity. The galaxy appears to be a relatively massive system, based on its size and brightness.
