The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge that is bright yellow. There is a slight elongation to the galaxy's shape, suggesting a mild deviation from a perfectly circular form. No distinct spiral arms or features are apparent. There may be some slight asymmetry in the outer edges of the galactic disk. The color suggests it is primarily composed of older stellar populations, implying that the star formation rate is low. No major mergers or disturbances are visible.
