This galaxy presents as a flattened, disk-shaped structure oriented nearly edge-on with respect to our line of sight. The central region exhibits a concentrated bulge, characterized by a yellowish-white hue, suggesting an older stellar population. The disk component displays a gradient in color, becoming bluer further from the center. A high fraction of its light is concentrated in the disk, though the bulge is still clearly visible. The galaxy does not appear to be undergoing a major merger, though there is some indication of possible tidal distortion or minor interaction. This system appears to be a fairly massive disk galaxy.