The galaxy presents a face-on spiral morphology, exhibiting well-defined spiral arms. These arms emanate from a central bulge, appearing moderately sized in relation to the overall galactic structure. The spiral arms display a somewhat tightly wound configuration, suggesting a developed stage of spiral structure. Two dominant arms are clearly discernible. The galaxy's disk is the predominant feature, with a relatively small contribution from the central bulge. There are no immediately obvious signs of major interactions or mergers, although some minor disturbances may be present. The presence of a bar feature cannot be ruled out but is not immediately obvious in this image, though it seems there is a weak bar present. The overall color profile suggests ongoing star formation.
