The galaxy presents a largely smooth, elliptical morphology.  It exhibits a centrally concentrated luminosity profile, with a gradual decrease in intensity towards the outer regions. The galaxy appears mostly featureless, with no discernable spiral arms or a prominent disk structure. Its color is generally blue, indicating a component of young, hot stars. The galaxy's apparent roundness suggests that we may be viewing it close to face-on. There is no obvious evidence of a major ongoing merger or tidal disruption.
