The galaxy appears to be a spiral galaxy, though the arms are not sharply defined. The disk exhibits a slight tilt relative to our line of sight. There is a suggestion of spiral structure, particularly on one side where it looks like the arms are winding outward. The central bulge appears small or non-existent, with a flattened disk profile. There are signs of ongoing star formation, with clumpy regions of bluer light present within the disk, suggesting active star-forming regions. There may be weak evidence of a bar feature crossing the galaxy's core. Also, there is some indication of potential merger activity or gravitational disturbance, with slight asymmetry in the overall disk structure. A fraction of the light appears reddish, which could suggest regions of older stellar populations or dust obscuration.
