The galaxy presents as an edge-on spiral, exhibiting a distinct disk structure. There appears to be a substantial central bulge, which shows a rounded morphology. The disk component is elongated and relatively smooth, with no immediately obvious spiral arm structures resolved in this image. The galaxy displays a color gradient, being brighter and more yellowish-white towards the central region, which could indicate a higher concentration of older stellar populations and dust obscuration. The outer disk appears fainter and slightly bluer, which may imply the presence of younger stars and active star formation regions, albeit not distinctly visible in this observation. The overall appearance suggests a relatively high inclination angle with respect to the observer's line of sight. Minor disturbances are present, but no major mergers are indicated.
