The galaxy presents as a spiral, observed at an angle that is neither perfectly face-on nor edge-on, exhibiting a moderate inclination. Two, possibly three, spiral arms are discernable. The spiral arms appear somewhat tightly wound. There is a distinct central bulge that does not appear to dominate the galaxy's overall structure. The color profile suggests a mix of stellar populations, with a yellower hue in the central bulge region likely indicating older, redder stars, while the spiral arms show hints of bluer regions, possibly indicative of ongoing star formation. The overall structure appears relatively undisturbed, although there is a slight asymmetry suggesting some interaction or past merger event. There is no sign of a strong central bar. The spiral arms are mottled rather than smooth, suggesting a clumpy distribution of star-forming regions.
