The galaxy exhibits a prominent disk structure, viewed at a moderate angle, but not perfectly edge-on. Spiral arms are clearly visible, displaying a morphology characterized by predominantly two spiral arms. These arms show a range of winding, from somewhat tightly wound to more loosely structured. The galaxy's central bulge appears moderately sized. There is indication of a bar feature bisecting the bulge, with a moderate to weak strength. Star formation is apparent, as indicated by regions of bluer light, concentrated primarily within the spiral arms. The overall shape is relatively undisturbed, though subtle asymmetries and minor disturbances may be present, but there are no obvious signs of major merger activity. The galaxy demonstrates a diverse stellar population, with regions of older, yellower stars concentrated in the bulge, and younger, bluer stars in the arms. The overall color profile suggests a significant population of intermediate to older stars.
