The galaxy presents as a centrally concentrated system with a smooth, largely featureless morphology. It exhibits a subtle but noticeable color gradient, appearing somewhat bluer in the outer regions and transitioning to a more yellow hue towards the core. The overall shape is elliptical, with a high degree of roundness, although there is a very slight elongation discernible. There is some evidence of gravitational disturbance, suggesting a possible ongoing or recent interaction. However, it is more likely that the galaxy is in the later stages of such an interaction. The bulk of the light appears to be emitted by an older stellar population, with a comparatively low rate of ongoing star formation. The galaxy is a relatively massive system, and displays an apparent lack of prominent spiral arms or a well-defined disk structure.
