The galaxy presents as a relatively smooth, elliptical structure with a concentrated central bulge. The core region exhibits a yellowish-white hue, suggesting an older stellar population dominating its composition. A subtle transition to a slightly bluer color is observed in the outer regions of the galaxy, possibly indicating the presence of a younger, star-forming population, though this activity seems subdued.

The overall shape appears more ovoid than perfectly circular, exhibiting a slight elongation. There are no prominent spiral arms or distinct features indicative of active galactic interactions. However, a faint, reddish, diffuse structure is noticeable, possibly indicative of a minor disturbance or tidal stream. The galaxy appears to be a quiescent system with minimal ongoing star formation.
