This galaxy presents as a relatively well-defined, elongated structure. The primary color of the galaxy appears to be a yellowish-orange hue, with hints of blue on the edges. This color distribution indicates possible differential stellar populations, with potentially older, redder stars concentrated in the central bulge, and bluer, younger stars in the disk.

The galaxy is moderately inclined from our line of sight, which allows some structural features to be seen. The galaxy appears to possess a disk-like structure and does not show any obvious signs of a spiral arm structure or bar. The relatively smooth appearance suggests the absence of a recent major merger event. There may be a slightly irregular feature in the disk, which may indicate minor tidal disturbances. 
