The galaxy presents a flattened elliptical morphology, appearing as a slightly elongated spheroid. The light distribution indicates a central bulge that is brighter and more concentrated. The galaxy's overall color appears to be consistent with an older stellar population, showing a yellowish hue at its center. Fainter, bluer regions may be present, though this is hard to be determined, in a disk-like structure.

No distinct spiral arms are observed. There are no obvious signs of active galactic nuclei activity or star formation. The edges of the galaxy blend into the background sky, without clear signs of tidal disruption or interaction with other galaxies. The galaxy exhibits a smooth light profile overall.
