The galaxy presents as a spiral galaxy with a notable disk structure that is not viewed edge-on. The galaxy exhibits distinct spiral arm features, with the structure displaying characteristics of tightly wound formations. The galaxy appears to be barred. There is a substantial bulge component. The galaxy is relatively isolated and does not appear to be undergoing any major merging activity or significant disturbances. The color gradients suggest ongoing star formation within the disk, particularly along the spiral arms. The overall luminosity indicates it is a relatively luminous galaxy.
