The galaxy exhibits a flattened, disk-like morphology, viewed at a significant inclination. A central bulge is apparent, exhibiting a concentrated luminosity profile with an orange hue, suggestive of an older stellar population. Fainter, bluish light emanates from the outer regions of the disk, possibly indicating younger star formation. There appear to be hints of spiral arm structure, though the inclination makes detailed observation difficult. The overall impression is of a galaxy undergoing active, but not excessively high, rates of star formation within its disk. The galaxy appears relatively undisturbed, showing no obvious signs of major mergers or tidal interactions.
