The galaxy presents as a slightly inclined, disk-shaped structure with an apparent smooth morphology. The central region exhibits a concentrated, yellowish-white glow, suggesting an older stellar population. The outer regions of the disk appear bluer, indicating the presence of younger, hotter stars. There is a faint suggestion of spiral arm structure, though it appears diffused rather than well-defined. The galaxy displays some signs of possible tidal disturbances or minor interactions, though no major disruptions are clearly visible. Overall, the galaxy appears to be a late-type spiral transitioning towards an earlier type or a disk galaxy with a significant bulge component.
