The galaxy appears as a relatively smooth, elliptical-like structure. It displays a concentrated central bulge that transitions outwards to a fainter, more diffuse halo. The color profile exhibits a trend of a more reddish hue in the central regions transitioning towards more green and blue tints in the outer regions. No obvious spiral arms or distinct dust lanes are discernible within the presented image. There seems to be no presence of any tidal disturbances or signs of recent or ongoing major mergers within the galaxy. The overall morphology suggests a galaxy that has undergone significant evolution with no clear disk structure, which indicates it may be of the elliptical or S0 type. 
