The galaxy appears as an elliptical-like structure with a smooth, centrally concentrated light profile. The object exhibits a generally spheroidal shape but appears somewhat elongated, showing a slight deviation from perfect circularity. The color gradients suggest a population of older stars, particularly towards the center. There is no obvious presence of spiral arms or distinct features indicative of active star formation. A fainter object is visible next to the primary galaxy, which may be a companion galaxy, but is likely interacting with the main galaxy. There does not appear to be any strong distortion of the morphology in either galaxy, meaning if they are interacting, it is either early or minor interaction. The lack of any distinct tidal tails or bridges connecting the galaxies indicates a merger is likely not occuring, but the closeness of the two galaxies suggests there could be a merger far in the future.