The galaxy presents a primarily smooth and rounded morphology. It exhibits a concentrated central bulge that appears golden in color, indicative of an older stellar population. The surrounding halo diffuses outwards with a subtle color gradient, transitioning from the warmer tones of the core to a cooler, greenish hue. There is no discernible spiral structure or dust lane visible in this image, suggesting a likely elliptical or lenticular classification. Faint extensions or tidal features are not obvious upon initial examination, implying no recent major merger events. There might be evidence of minor disturbances present, but the overall structure appears relatively undisturbed.
