The galaxy presents as a relatively smooth and rounded structure. It exhibits a centrally concentrated light profile, appearing brightest at its core, which is consistent with a bulge-dominated morphology. A subtle color gradient is observed, transitioning from a bluer hue at the center to slightly redder tones in the outer regions, suggesting potential variations in stellar populations or dust content across the galaxy. No obvious spiral arm structures or prominent dust lanes are discernible in this image. There is no evidence of any significant tidal disturbances or ongoing major mergers with other galaxies. Overall, the galaxy appears to be an undisturbed, early-type system with a well-defined elliptical shape.
