The galaxy presents as a relatively compact, elliptical-like structure. It appears generally smooth in texture, exhibiting a high degree of rotational symmetry with little evidence of prominent spiral arms or significant disk features. The core of the galaxy is noticeably brighter and more concentrated, indicative of a significant concentration of stars.

There is some indication of a slight disturbance within the galaxy, potentially a minor interaction or faint tidal feature, though overall the structure is fairly regular. The color of the galaxy appears relatively uniform across its body. The galaxy may be undergoing a low level of star formation.
