The galaxy appears as a slightly elongated, disk-like system, seen at an oblique angle, but not quite edge-on. The central bulge is moderately prominent, exhibiting a smooth, concentrated light distribution, suggesting an older stellar population. The disk component shows hints of spiral structure, with subtle color variations indicating the presence of younger, bluer stars in some regions. There are also areas of dust obscuration in the disk, which contribute to the irregular appearance. The overall color of the galaxy is moderately blue, suggesting ongoing star formation. The outer regions of the galaxy appear somewhat diffuse, and the isophotes become less distinct as the light fades into the background sky. There may be some minor tidal disturbances or interactions, but no significant, large-scale merging activity is evident.
