The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated central bulge with a diffuse, extended halo. The color profile suggests an older stellar population, dominated by redder wavelengths with a comparatively subdued contribution from blue wavelengths. There is a notable lack of distinct spiral arm structures or prominent dust lanes. The overall structure appears largely undisturbed, indicative of a gravitationally settled system without significant ongoing merger activity. The galaxy appears nearly spherical. The smooth and rounded appearance indicates that the system is likely relatively evolved and quiescent in terms of star formation.
