The galaxy presents a generally elliptical morphology with a smooth, centrally concentrated light distribution. The core appears relatively bright and yellowish-orange, gradually fading to a greenish hue at the outskirts. No distinct spiral arms or prominent dust lanes are discernible, suggesting a lack of ongoing major star formation. The overall structure exhibits a high degree of symmetry and roundness, with no evidence of significant tidal disturbances or ongoing merger activity. Given these characteristics, the galaxy appears to be a relatively massive, quiescent elliptical galaxy.
