The galaxy presents as an edge-on spiral, with a clearly defined central bulge exhibiting a yellowish-white hue, indicative of an older stellar population. The disk component, viewed nearly edge-on, appears flattened and extended, showing a bluer color, suggesting the presence of younger, hotter stars and ongoing star formation within the spiral arms. There appears to be a slight warping of the disk. There is no obvious active galactic nucleus. There is no indication of a major ongoing merger. There may be some minor tidal disturbances.
