The galaxy appears to be a relatively smooth, centrally concentrated object, likely an elliptical or lenticular galaxy given the lack of prominent spiral arms or a well-defined disk. It exhibits a moderate degree of roundness, with a subtle elongation that prevents it from being perfectly circular. There are hints of color variation within the galaxy, with a reddish-orange hue dominating the central region, potentially indicating an older stellar population. The outer regions show hints of bluer colors, which would suggest ongoing or recent star formation in those areas. The galaxy shows no major signs of a merger and only minor signs of disturbance. The galaxy is moderately luminous.