The galaxy presents as a disk galaxy, seen nearly edge-on. A prominent central bulge is observed, appearing more luminous than the surrounding disk. The disk itself exhibits a flattened, elongated structure. The galaxy displays a smooth overall appearance, with no distinct spiral arm features immediately apparent, likely due to its edge-on orientation. Color gradients are subtle, with the bulge tending toward yellow-orange hues, possibly indicative of an older stellar population. The disk appears slightly bluer, suggesting the presence of younger, hotter stars. The outer regions of the disk gradually fade into the background, making precise measurements of its total extent difficult. There is no obvious sign of ongoing major mergers.
