The galaxy appears as a moderately bright, elliptical-shaped structure. Its core exhibits a concentrated luminosity, appearing almost spherical. The intensity of the light decreases gradually outwards from the core, forming a diffuse halo. The galaxy is elongated, with the major axis notably longer than the minor axis, giving it a slightly cigar-shaped appearance. There are no visible spiral arms or distinct dust lanes. The overall color is a yellowish-white, suggesting an older stellar population with minimal ongoing star formation. The smoothness of its light distribution indicates that it is likely an elliptical galaxy that has undergone limited recent interactions or mergers.
