The galaxy presents a smooth, elliptical morphology with a notable central bulge that dominates the overall structure. The light distribution appears relatively uniform, lacking prominent spiral arms or distinct features typically associated with disk galaxies. There is a slight elongation in shape, suggesting a transition between perfectly spherical and a more cigar-shaped form. A faint, diffuse halo surrounds the brighter central region, indicating a gradual decrease in stellar density with increasing distance from the galactic core. The galaxy's color appears to be a yellow-red hue, possibly indicating a population of older stars. There is no clear evidence of active star formation regions or significant dust lanes visible in this image. There are no signs of major disturbances. The galaxy appears to be relatively isolated.
