The galaxy presents as a somewhat smooth, elongated structure with a cigar-like shape. A concentration of light is observed in the central region, suggesting a prominent galactic bulge or core. The galaxy exhibits a color gradient, transitioning from a yellower hue in the center to a bluer tint towards its outer edges. The overall morphology suggests the possibility of an elliptical galaxy or a spiral galaxy viewed edge-on, lacking defined spiral arms. There may be evidence of ongoing star formation, particularly in the outer regions, indicated by the bluer color. The galaxy appears relatively undisturbed, showing no clear signs of major merging events. Minor disturbances are possible, but not definitively discernible from this image.
