This galaxy appears to be a relatively smooth, elliptical system. The central bulge exhibits a distinct reddish hue, likely indicating an older stellar population with lower rates of star formation. Surrounding the core, a more diffuse, blueish halo is visible. This halo suggests the presence of a younger, bluer stellar population, indicative of ongoing or recent star formation. The galaxy appears largely undisturbed, showing no strong signs of tidal interactions or major mergers, although minor disturbances cannot be ruled out given the slight asymmetry observed in the outer regions. It has a generally rounded morphology, with no apparent disk structure.
