This galaxy exhibits a distinct spiral structure. The arms are well-defined and extend outward from a central bulge. The bulge appears to be of moderate size, neither excessively large nor particularly small, and possesses a yellowish hue, possibly indicative of an older stellar population. The spiral arms show evidence of active star formation, as indicated by their bluish color, which suggests the presence of hot, young stars. The winding of the spiral arms is somewhat varied; sections appear moderately wound, while others are more loosely defined. There is a possibility of a bar structure, but the image resolution makes it difficult to confirm. The galaxy does not show any obvious signs of significant merging activity, but some minor disturbances in the disk could be present. A faint, extended halo appears to surround the main disk structure.
