The galaxy appears to be a spiral galaxy, exhibiting a prominent disk structure. Evidence of spiral arms are present within the disk, although the resolution limits the precise tracing of their morphology. The central bulge is clearly visible, displaying a moderate size relative to the disk. There is a bar structure present within the central region. The color profile suggests active star formation regions within the disk, characterized by a bluer hue, whereas the bulge appears to be more composed of older stellar populations, shown by the yellow-reddish hue. The galaxy appears somewhat disturbed, potentially indicating interactions or mergers.
