The galaxy presents a generally smooth morphology, appearing as a concentrated spheroid with a notable central bulge. The light distribution suggests a high degree of radial symmetry, with isophotes that are predominantly elliptical. The primary color observed is a yellow-orange hue, which could indicate an older stellar population dominating the light output. There is faint suggestion of bluer light in the outer regions which may indicate low levels of star formation. There are no clear indications of spiral arms, a bar structure, or other prominent disk features. The galaxy appears relatively undisturbed, with no major signs of tidal interactions or ongoing mergers.
