The galaxy appears as a centrally concentrated object with a generally smooth morphology. Its shape approximates an elliptical form, showing a slight elongation rather than being perfectly circular. The galaxy exhibits a color gradient, transitioning from a warmer, reddish hue towards the center to a cooler, greenish-blue towards the outer regions. This may indicate differing stellar populations or dust distribution within the galaxy. While the overall structure is smooth, there is a hint of some internal irregularity or minor perturbation, possibly suggesting a past or ongoing minor interaction. No obvious signs of spiral arms or a well-defined disk are discernible.
