The galaxy appears as a relatively small, disk-shaped system, presented nearly edge-on to our line of sight. There is evidence of a central bulge, though it is not particularly prominent. The disk exhibits a bluer hue, suggestive of ongoing star formation. The galaxy lacks a strongly defined spiral structure, appearing more like a lenticular galaxy. Faint dust lanes appear near the center, attenuating light along the disk. There's no obvious interaction with any nearby galaxies and no apparent major disturbances.
