The galaxy presents as a relatively smooth, elliptical structure with a high degree of central concentration. Its overall color appears yellowish, suggesting an older stellar population with a diminished rate of ongoing star formation. The galaxy's shape is not perfectly circular; it exhibits a noticeable elongation, with the major axis extending approximately northwest to southeast. The surface brightness profile appears to be well-fit by a Sersic profile with a high Sersic index, reinforcing the notion of a bulge-dominated morphology with little disk component. There is no obvious presence of spiral arms or dust lanes. Minor disturbances may be present, or this galaxy may be in the process of merging, though these are difficult to fully resolve. The color gradients seem to be shallow, with the core only slightly more chromatic than the edges.
