The observed galaxy exhibits a distinct disk morphology, with a relatively faint but visible structure suggesting spiral arms. These arms appear somewhat clumpy and not tightly wound. There is also a noticeable bar feature that is somewhat obscured. The galaxy's color profile indicates active star formation within the disk, particularly along the spiral arms, with a blue hue evident in these regions. The image suggests there may be ongoing or recent interactions or merger events with another galaxy, as the shape of the galaxy is somewhat asymmetric and distorted. The central bulge is small or non-existent, indicating that this is a spiral galaxy.
