The galaxy presents as a spiral galaxy with a prominent disk structure. The spiral arms appear somewhat loosely wound. Two main arms are easily discernible, originating near the central bulge and extending outwards. There appears to be active star formation occurring along the spiral arms, as indicated by the presence of bluer regions. The central bulge region exhibits a yellower/redder hue, which could indicate an older stellar population. The galaxy is not perfectly face-on, as there's a slight tilt that gives a sense of depth to the spiral structure. The disk does not appear to be perfectly symmetrical, potentially indicating some gravitational interaction or past merging event. There may be a bar structure in the central region. The galaxy is not completely isolated, given the disturbances in the arms. There is evidence of potential minor disturbances throughout the galaxy.