The galaxy exhibits a spiral morphology, with a dominant, but not overwhelming, disk component. The spiral arms are prominent and well-defined, extending outwards from a central bulge. The bulge appears moderately sized. There is no strong evidence of a bar structure in the central region. The galaxy displays a relatively smooth appearance overall, suggesting a lack of significant recent major merger events. There may be minor disturbances in the structure, which is difficult to say based on the resolution of the image. The galaxy is face-on. The color distribution suggests active star formation is present, though not at an extremely high rate.
