The galaxy presents as a spiral, although the structure is somewhat flocculent. Tightly wound spiral arms emanate from a central bulge, extending into the galactic disk. A prominent, moderately luminous core is visible at the galaxy's center, characteristic of a central bulge. There is a hint of a bar feature in the galaxy's center, although it's not very prominent. The galaxy exhibits blue-ish tones in its arms indicating ongoing star formation, but does not appear to be exceptionally active. There is not much dust obscuring the galaxy disk. It appears relatively undisturbed, not showing significant signs of major mergers or tidal interactions, although minor disturbances cannot be ruled out. The galaxy displays a moderate inclination relative to our line of sight; it is not viewed edge-on, but nor is it perfectly face-on. Overall the morphology is consistent with that of a typical spiral galaxy, exhibiting both bulge and disk components, and evidence of relatively recent star formation within the spiral arms.
