This galaxy appears to be a relatively smooth, elliptical-like system with a concentrated central bulge. The light profile suggests a high degree of sphericity. The central region exhibits a yellowish hue, potentially indicating an older stellar population. Moving outward from the core, the galaxy displays a gradual decrease in brightness. There's an area of bluer light mixed within the outer halo regions on the left, which may indicate an area of star formation. Possible minor tidal disturbance evident in the form of an extension of the galaxy on the upper right edge. Overall, the morphology suggests a galaxy that is relatively undisturbed, with an estimate of relatively high mass.
