The galaxy presents as a largely smooth, elliptical-like structure. It exhibits a concentrated, bright core that appears yellowish-white in color, indicative of an older stellar population. The isophotes, while somewhat indistinct due to image resolution, seem generally rounded, trending towards elliptical rather than a highly flattened disk. There's no clear evidence of spiral arms or a significant dust lane within the galaxy's visible structure. Faint extensions of diffuse light surround the central region, creating a more ill-defined halo. The overall color suggests a lack of significant ongoing star formation in the bulk of the galaxy, although it cannot be ruled out in the outskirt regions. The general undisturbed morphology indicates no recent major merger events.
