The galaxy presents as a moderately bright, elliptical-like structure with a smooth, concentrated light profile. It appears somewhat elongated, deviating slightly from a perfectly circular shape. The central region exhibits a higher surface brightness, suggesting a concentration of older stellar populations, likely redder in color. The outer regions fade gradually into the background sky, indicative of a decreasing stellar density. There is no apparent evidence of spiral arms or distinct dust lanes. Overall, the galaxy's morphology is relatively undisturbed, without any obvious signs of ongoing major mergers or tidal interactions. The overall color seems to be slightly leaning to the redder end of the spectrum.
