This galaxy presents an elliptical morphology, exhibiting a smooth light distribution and a high degree of central concentration. The overall color appears yellowish-orange, suggestive of an older stellar population with fewer young, massive stars.

The galaxy displays a relatively undisturbed structure; however, a possible minor interaction with a small nearby object is suspected, which may be a companion galaxy. A faint tidal stream or bridge of material may also be seen connecting the two. There is no evidence of spiral arms or a prominent disk.

The estimated angular size is small, indicating a considerable distance. Its absolute magnitude suggests a very luminous system, likely housing a large stellar mass and possibly a supermassive black hole at its core. The galaxy is currently undergoing a low rate of star formation.
