The galaxy presents as a spiral type, exhibiting a disk-like structure. It is primarily oriented face-on, with a noticeable central bulge. The spiral arms are prominent, extending outwards from the central bulge. There are a possible two distinct spiral arms, indicating a bisymmetric structure. These arms appear moderately wound. There is evidence of a bar-like structure running through the central region. The central bulge seems relatively small compared to the overall disk size. There is a suggestion of minor tidal disturbance and a small merging partner. The overall color appears to be dominated by blue hues, with an orange center, implying moderate star formation activity.
