The galaxy presents as a smooth, centrally concentrated object, exhibiting a subtle reddish hue. It lacks any readily discernible spiral arm structure or distinct features. The morphology appears largely spheroidal or elliptical, with a high degree of symmetry. The object shows no obvious signs of ongoing major merger activity, such as tidal tails or significantly distorted isophotes, although minor disturbances cannot be ruled out at this resolution. Based on the color profile, the galaxy likely exhibits a relatively low current star formation rate.
