The galaxy presents as a relatively compact and somewhat elliptical-shaped object. The light is primarily concentrated in a central bulge, appearing smooth and without significant substructure in the image resolution. The galaxy exhibits a subtle colour gradient, appearing slightly bluer towards the central regions and redder towards the periphery. The overall luminosity suggests a substantial stellar mass. There is no prominent spiral arm structure or dust lanes visible. There are some disturbances suggesting the possibility of a minor merger.
