This galaxy exhibits a pronounced central bulge, indicating a concentration of older stars. The bulge is a yellowish-white hue, and the surrounding disc structure appears relatively smooth with a blue tinge. This suggests a combination of older stellar populations in the bulge and more recent star formation in the disc. The galaxy does not exhibit strong spiral arm features. There is a slight asymmetry, with the blue star formation appearing more pronounced in the lower left portion of the disc relative to the upper right. No dust lanes or evidence of tidal interactions are apparent. The galaxy appears to be isolated. The overall impression is of a spiral galaxy with a dominant bulge, moderate star formation, and no immediately obvious signs of recent mergers or major disturbances.
