The galaxy presents as a roughly elliptical-shaped object. The morphology indicates a significant smooth component, with a more amorphous, less defined structure. A central, bright region is visible, likely a galactic bulge. The galaxy exhibits a color gradient, transitioning from a bluer hue on the outer edges to a redder, more concentrated core. The color suggests older stellar populations dominate with lower levels of on-going star formation. There is some evidence of possible disturbance or tidal interactions.
