This galaxy appears to be a spiral galaxy exhibiting a well-defined disk structure. Two prominent spiral arms emanate from the central bulge, displaying a moderately loose winding pattern. The central bulge seems relatively large, with a color indicating an older stellar population. Star formation appears active within the spiral arms, evidenced by the slightly bluer hues in those regions compared to the bulge. There's no obvious sign of a strong bar feature bisecting the galaxy, though a subtle elongation could indicate a weak bar presence. The galaxy does not appear to be undergoing any major merging activity, although there is a possibility of some minor disturbance in the outer regions of the disk.
