The galaxy presents as a smooth, elongated structure with a dominant, bright central bulge that fades in color toward the less defined edges. The galaxy appears cigar-shaped, lacking defined spiral arms or distinct morphological features, possibly indicative of an elliptical or lenticular galaxy type. It exhibits a color gradient transitioning from a yellowish core to a bluer, fainter halo. There is no visually apparent interaction or major disturbance to suggest a recent merger event, though minor disturbances cannot be ruled out. Overall, the galaxy appears relatively isolated and undisturbed.
