The galaxy presents as a spiral type, exhibiting a prominent central bulge that appears yellowish in color, suggesting an older stellar population. The spiral arms are well-defined, tracing a grand design morphology and are wound moderately tightly around the galactic center. Two main arms are discernible. They appear slightly bluer compared to the bulge, indicating regions of ongoing star formation. There is subtle evidence of a bar structure traversing the central region of the galaxy, although it is not particularly strong. The disk is oriented at an angle relative to our line of sight, allowing a partial view of the spiral structure. Overall, the galaxy appears relatively undisturbed, with no major signs of ongoing mergers or tidal interactions.
