The galaxy is a disk galaxy, viewed nearly edge-on. The central bulge is prominent, exhibiting a color gradient suggesting an older stellar population. It is elongated, appearing mostly rounded, and dominates the galaxy's core region. The disk itself is thin and exhibits a noticeable dust lane that obscures some of the light from behind it. There appears to be only very minor asymmetry or perturbation in the disk, suggesting minimal ongoing or recent merger activity. Overall, the galaxy appears smooth with a weak disk structure.