This galaxy exhibits a clear spiral structure. The spiral arms are well-defined, extending from a bright, moderately sized central bulge. A prominent bar feature appears to bisect the bulge along its major axis. The arms are wound relatively tightly with some of the spiral arms appearing more distinct than others. Some regions within the disk and surrounding the spiral arms show areas with a clumpy structure which could possibly indicate some minor disturbances. The light distribution within the galaxy varies, suggesting differential stellar populations or dust obscuration. The colors observed suggest star formation is occurring. Overall the morphology points to a barred spiral galaxy with potential ongoing interactions or internal dynamics influencing its structure.
