The galaxy appears as a centrally concentrated, smooth object. It exhibits a generally elliptical morphology with a high degree of central symmetry. The light distribution is relatively uniform across the galaxy, lacking distinct spiral arms or pronounced features typically associated with disk galaxies. A slight color gradient is observed, with a central region displaying a subtle reddish hue, transitioning to a bluer tint toward the outer regions. This may indicate some ongoing star formation in the galaxy. There is no evidence of any major mergers or tidal disturbances in the image.
