This galaxy appears to be a spiral galaxy, not viewed edge-on. It exhibits a disk-like structure, with a slight inclination relative to our line of sight. The central bulge appears prominent and relatively smooth. Faint spiral arm features are visible in the surrounding disk. The galaxy displays varying colors across its structure, with a bluish hue indicating regions of younger, hotter stars within the spiral arms and a redder color toward the bulge, potentially indicating an older stellar population. There are some disturbances present, possibly indicating minor interactions with other galaxies, however it's more likely that the galaxy isn't perfectly relaxed and is undergoing some sort of internal process leading to these morphological features. The star formation rate, though not high, is still present, suggesting continued stellar evolution within this system.
