The galaxy presents a predominantly smooth morphology. The light distribution is centrally concentrated with a bright core region. The galaxy appears largely elliptical with a high degree of roundness. There is no evidence of strong spiral arm structure or significant disk features visible in the image. A slight deviation from perfect ellipticity is observed, though no distinct tidal tails or merger features are clearly present. The object exhibits a color gradient, transitioning from a yellowish central region to a bluer outer halo, suggesting a population gradient with older stars concentrated in the center. Star formation appears to be low.
