This galaxy exhibits a morphology that appears to be a disk galaxy, viewed at an oblique angle. The central region shows a high concentration of light, suggestive of a significant bulge component. This bulge appears yellow-ish, indicating an older stellar population, possibly dominated by red giant stars. Fainter, bluer regions are visible extending from this central region, suggesting the presence of younger, star-forming regions, although these features aren't very distinct. Some asymmetry is seen in the outer disk, which could indicate minor tidal disturbances. There is a blueish object in the top-right that could indicate either a strong star forming region, or an area that has been affected by a tidal interaction. The overall structure does not exhibit any significant merging activity, but there may have been minor gravitational disturbances that have affected the shape of the disk. The galaxy exhibits a relatively smooth texture.
