The galaxy presents as a somewhat rounded structure with a smooth appearance, lacking any obvious spiral arms or distinct features generally associated with disk galaxies. There is a noticeable color gradient from the center outward. The central region exhibits a yellowish hue, suggesting a population of older stars and potentially a lower rate of ongoing star formation. Moving outwards, the color shifts slightly towards a redder tone. Based on the smoothness and roundness, it is probably an elliptical galaxy. The galaxy appears to be isolated, with no signs of interaction with other galaxies or major disturbances in its structure. A small region below the galaxy seems to exhibit recent star formation.
