The galaxy presents as a highly inclined, possibly edge-on, disk galaxy. There is an indication of a central bulge, exhibiting a somewhat rounded morphology. The galaxy displays a smooth appearance, though there might be underlying disk structures. The color gradient suggests a slightly bluer disk and a redder bulge, possibly indicating ongoing star formation within the disk. There is no readily apparent sign of major disturbances, mergers, or tidal features. The galaxy does seem somewhat symmetrical in shape, which further suggests it is not currently undergoing a major merging event.
