The galaxy appears to be a spiral galaxy viewed at a significant inclination. The central bulge is prominent and exhibits a yellowish-white hue, suggesting an older stellar population and a lack of significant ongoing star formation. The spiral arms are visible, though not sharply defined, displaying a bluer color, indicative of younger, hotter stars and regions of active star formation. The arms appear somewhat patchy and flocculent, suggesting a less grand-design spiral structure. There's a slight asymmetry in the distribution of light within the disk, potentially indicating a minor interaction or disturbance. Overall, the galaxy presents a moderate level of star formation activity and an estimated mass range of 10^10 solar masses.
