The galaxy appears as a slightly elongated, cigar-shaped object with a smooth, diffuse light distribution. There is a distinct central bulge that gradually fades into the outer regions of the galaxy. The galaxy exhibits a subtle color gradient, appearing slightly bluer towards the central region. No obvious spiral arm structures or dust lanes are discernible, suggesting a relatively smooth stellar population. The general morphology implies that this is likely a disk galaxy that is seen from an angle. There are no obvious signs of ongoing mergers or major disturbances. The galaxy's overall appearance suggests that it is in a relatively quiescent state of star formation.
