The galaxy appears to be a spiral galaxy, viewed at a slight angle such that it is nearly face-on. Two prominent spiral arms are visible, originating from the central bulge and extending outwards. The winding of these arms appears moderate, and extend outwards significantly. The central bulge region presents a moderate concentration of light. There may also be a weak bar structure present, although this is difficult to discern with certainty. The color of the galaxy indicates active star formation, especially in the spiral arms. There are no indications of strong tidal disturbances or major mergers; however, there may be minor disturbances. The overall structure suggests a relatively unperturbed spiral galaxy, consistent with ongoing star formation and the presence of distinct spiral arms.