The galaxy presents as a smooth, centrally concentrated object with an elliptical morphology. The core exhibits a bright, diffuse glow, suggesting a significant population of older stars. Fainter, less defined disk-like structure appears at the outer edges, with subtle color variations. These color gradients suggest a slightly bluer stellar population within the outer regions compared to the core. The overall appearance is consistent with an early-type galaxy, potentially an elliptical or lenticular galaxy, with only slight indications of disturbance to its structure.
