The galaxy presents a discernible disk structure, though its orientation relative to our line of sight makes detailed analysis challenging. The disk appears not to be viewed edge-on. Spiral arms are clearly visible, exhibiting a well-defined morphology. There is no apparent bar structure. The central bulge region has a yellow hue and appears moderately sized relative to the overall dimensions of the galactic disk. The outer regions of the galaxy exhibit a blue tinge, suggestive of ongoing star formation. The galaxy appears relatively undisturbed, with no immediate signs of a major merger event or significant tidal distortions. Minor disturbances may be present, but are difficult to discern at this resolution.
