The galaxy presents as a spiral galaxy, viewed at a relatively high inclination. The central bulge is prominent and appears moderately sized, with a yellowish hue indicating an older stellar population. Spiral arms are visible and traced by pockets of bluer light, suggesting ongoing star formation. The arms are somewhat flocculent in appearance and can be traced along a majority of the galaxy's span. No obvious major merging events are occurring, though some minor disturbances cannot be ruled out in the outer reaches of the disk. A weak or absent bar is likely. The galaxy's morphology is predominantly disk-like rather than purely elliptical.
