This galaxy appears to be a spiral galaxy viewed at a moderate inclination. It exhibits a prominent central bulge with a yellowish hue, suggesting an older stellar population. The spiral arms are clearly defined, predominantly featuring moderate winding. These arms display a bluish color, indicating the presence of younger, hotter stars and ongoing star formation. There may be a bar feature at the center of the galaxy. The galaxy does not appear to be undergoing any major merging events or significant tidal disturbances. Based on its morphology, the galaxy is likely actively forming stars.
