The galaxy presents as a relatively smooth, elliptical-like object with a concentrated central bulge. The color profile indicates an older stellar population, with a dominant yellowish-orange hue. There's a subtle elongation, though it appears more rounded than cigar-shaped. No distinct spiral arm structures or prominent dust lanes are apparent. The overall morphology suggests minimal recent or ongoing merger activity, displaying a largely undisturbed structure. The galaxy is moderately luminous, indicative of a substantial stellar mass, yet shows a low rate of star formation.
