The galaxy appears to be an elliptical galaxy, exhibiting a smooth, featureless morphology. The light distribution suggests a high degree of spherical symmetry, though a slight elongation is observed along one axis. The galaxy's central region displays a high surface brightness, indicating a concentrated stellar population. The color profile is relatively uniform, transitioning from a slightly bluer hue in the outer regions to a redder color towards the core. There is no visual evidence of spiral arms, a prominent disk, or active star formation. The overall appearance points to an older stellar population, consistent with a passively evolving system. There are no signs of a recent major merger event or significant tidal disturbances.
