The galaxy presents as a generally smooth, elliptical morphology with a high degree of central concentration. The light profile appears to gradually decrease in intensity from the core outwards, with no apparent substructure or spiral arms visible in this imaging. The axial ratio suggests a moderately elongated shape, deviating slightly from perfect sphericity. The dominant color is yellowish-orange, indicating an older stellar population. The light in the central region is noticeably brighter than that of the galaxy's outer edges. There is a faint hint of blue in the furthest edges of the galaxy which may indicate some more recent star formation. No signs of active galactic nuclei or strong tidal interactions are readily apparent in the image. Overall, the galaxy appears relatively undisturbed.
