The object appears to be a spiral galaxy with a significant bulge component. Two prominent spiral arms emanate from the central region, exhibiting a tightly wound structure. The color profile suggests ongoing star formation, particularly within the arms, indicated by their bluish hue. The arms themselves display a degree of patchiness, suggesting the presence of numerous star-forming regions. While the image resolution limits detailed morphological analysis, there is potential indication of a bar structure across the central region of the galaxy. No signs of major mergers or extreme disturbances are immediately apparent, though minor tidal features cannot be ruled out. The central bulge presents with a yellowish-orange color, indicative of an older stellar population.