The galaxy presents as a spiral galaxy with a moderately inclined disk. The spiral arms are well-defined and appear tightly wound, exhibiting a distinct pattern. The color gradient suggests a central bulge region with a yellowish hue, which could indicate a population of older, redder stars. The outer disk appears bluer, possibly due to the presence of younger, hotter stars and ongoing star formation. The galaxy exhibits a prominent disk with a small bulge. The morphology is largely undisturbed, lacking significant signs of mergers or tidal interactions.
