This galaxy exhibits a spiral morphology, characterized by a prominent central bulge surrounded by a disk. The disk shows clear spiral arm structure, with two main arms being the most easily identifiable. These arms appear to be moderately wound, not tightly wrapped around the nucleus. The presence of a bar is suspected, although it is not definitively clear. The bulge appears to be of moderate size, with the disk being more dominant in overall size. There is evidence of possible interaction or disturbance present within the structure of the galaxy, particularly around the edges of the disk. It appears that this galaxy might be undergoing or have recently undergone a minor merger or interaction event with another galaxy. The colors appear to be bluer in the spiral arms, potentially indicating ongoing star formation within the galaxy.
