The galaxy presents as a flattened spheroid, likely an elliptical galaxy, with a smooth, diffuse light distribution. The core region exhibits a concentrated, brighter orange hue, suggesting a population of older stars dominating the central region. Moving outwards from the core, a subtle shift towards bluer tones is observed in the surrounding halo. The halo appears relatively homogenous. There is no strong visual evidence of distinct spiral arms or significant dust lanes. Minor disturbances are possibly present but not easily discernible. Overall, the galaxy has a settled, relatively undisturbed morphology.
