This galaxy appears to be a spiral galaxy viewed at a moderately inclined angle. The central bulge is bright and concentrated, with a noticeable flattening towards the outer regions. The spiral arms are somewhat flocculent and not as tightly wound. There's evidence of active star formation within the arms, indicated by the patchy blue regions. A slight asymmetry is observed on one side of the galaxy, possibly hinting at minor gravitational interaction or recent accretion events. Overall, the galaxy presents a well-defined disk structure with ongoing star formation.
