The galaxy presents as a moderately bright, elliptical structure with a high degree of central concentration. The core region exhibits a bright, unresolved nucleus. Moving outward, the light gradually decreases, and the overall color appears to become slightly bluer toward the edges.

The galaxy appears largely smooth in texture. There is no evidence of strong spiral arm features or dust lanes. Faint hints of possible tidal disturbances are visible, but these could also be artifacts of observation. A slight elongation is observed, giving it a shape somewhere between circular and cigar-shaped. The galaxy is likely experiencing a relatively low rate of star formation, considering its morphology and color profile.
