The galaxy presents as a face-on spiral. Its morphology is characterized by well-defined spiral arms emanating from a moderately bright central bulge. The spiral arms exhibit a tightly wound structure, displaying a clear multi-arm pattern. The arms are not entirely uniform in color, showing variations indicative of differing stellar populations and star formation activity. The central bulge is subtly elongated, possibly hinting at the presence of a weak bar structure. There are signs of possible ongoing or recent star formation, as implied by regions of bluer light within the spiral arms. There is no evidence of a major merger event, although some minor irregularities in the arm structure could suggest past interactions. The overall structure suggests a spiral galaxy in a relatively quiescent state of evolution.
