The galaxy appears as a flattened, disk-shaped system viewed nearly edge-on. The central bulge is prominent and exhibits a smooth, yellowish color, suggestive of an older stellar population. The disk itself is relatively thin and elongated, with a slight warping or flaring visible. The color gradients within the disk are subtle, but a slightly bluer hue may be present in the outermost regions, hinting at ongoing star formation. No distinct spiral arm structure is discernible. The galaxy exhibits no obvious signs of a recent major merger or tidal disturbances, though some minor irregularities in the disk morphology cannot be ruled out. The overall appearance suggests a relatively evolved spiral or lenticular galaxy with a substantial stellar mass.
