The galaxy presents a clear disk structure, oriented approximately edge-on relative to our line of sight. A prominent central bulge is observed, exhibiting a smooth, concentrated luminosity profile. The bulge appears to be moderate in size compared to the overall disk. The galactic disk displays subtle hints of spiral arm structure, though the near edge-on orientation makes detailed tracing difficult. These spiral arms are somewhat indistinct and patchy, not clearly defined. There is no obvious major merging event taking place, though some minor asymmetry or disturbances in the outer disk cannot be ruled out. A bar is likely present traversing the central region, showing hints of a moderately strong bar-like structure. The galaxy displays a color gradient, with a more yellowish hue in the central bulge, suggestive of an older stellar population, and bluer tones in the disk, indicative of ongoing star formation.
