The galaxy presents as a spiral type, with a notable bulge and a well-defined disk structure. The spiral arms appear tightly wound around the central bulge. Evidence suggests the presence of two or more spiral arms. A weak bar-like structure may be present in the central region. The bulge exhibits a moderate size relative to the overall disk. There is no strong evidence of ongoing major mergers, although subtle signs of minor disturbance are present, suggesting potential interactions with smaller companion galaxies. The galaxy's orientation presents a face-on view, allowing a clear view of the spiral structure. The color profile indicates ongoing star formation activity within the spiral arms, as indicated by the blue hues in the arms and the more yellow hues in the bulge.
