The galaxy appears to be a relatively smooth, centrally concentrated object. It exhibits a radial color gradient, trending from a bluer, possibly actively star-forming core region to redder outer regions. The central bulge exhibits high luminosity, and the galaxy appears to be elliptical in shape, with only a slight ellipticity observed. There is no strong evidence of spiral arm structures, but there seems to be a slight disk-like feature. No signs of any major merger events or galactic disturbances can be seen. 
