The galaxy presents as a relatively smooth and elliptical structure. The central region displays a concentrated luminosity with a yellowish-white hue, suggesting an older stellar population. Moving outwards from the core, the color transitions into a reddish, then bluish band. The color suggests the presents of dust lanes and regions of more recent star formation. The galaxy exhibits a cigar shape, indicating that the galaxy is not perfectly spherical and that we are potentially viewing it at an angle. There are no obvious signs of a major ongoing merger or tidal disturbances, although minor irregularities may be present. The overall morphology suggests a galaxy that has undergone significant evolution and is currently relatively quiescent.
