The galaxy presents as a relatively smooth, elliptical-like structure with a bright, concentrated central bulge. The overall color profile indicates a predominantly older stellar population, suggested by the yellowish-red hue. There is a slight elongation to the galaxy's shape, with the major axis oriented in a roughly northeast-southwest direction. No distinct spiral arms or prominent dust lanes are discernible. A very faint halo or extended envelope is subtly apparent surrounding the main body, gradually fading into the background sky. There is a possibility of minor disturbances, which suggest recent or ongoing interactions with smaller galaxies or gas clouds, but it is difficult to say for certain without high-resolution imaging.
