The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge that appears almost spherical. The light distribution fades gradually from the core outwards, with no discernible spiral arm structures or distinct features. The color is predominantly a pale yellow-white, suggesting an older stellar population with minimal ongoing star formation. There may be very subtle signs of minor disturbances, but no major merging events are apparent in the image. The galaxy appears generally isolated and undisturbed.
