The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology appears largely spheroidal with a high degree of roundness. There is little evidence of spiral arm structure or significant disk features. The galaxy exhibits a color gradient, with a brighter, bluer core gradually transitioning to a redder outer halo. Some minor disturbances could be occurring within the galactic structure. The estimated size would indicate that this galaxy is typical for its type. This galaxy may be undergoing active star formation.
