The galaxy presents as a relatively smooth, elliptical-like structure, with a concentration of light towards the center. The shape appears largely round, with only slight deviations from perfect circularity. A faint, diffuse halo seems to surround the brighter central region, gradually fading into the background sky. There's no obvious evidence of spiral arms or a prominent disk component. The galaxy's color is primarily yellowish-orange, suggesting a population of older stars. There are subtle indications of some irregularities in the light distribution, hinting at the possibility of a minor disturbance or interaction with a smaller companion, though no significant merger activity is immediately apparent.
