The galaxy appears as a disk-shaped structure, oriented edge-on relative to our line of sight. A central bulge is visible, characterized by a brighter, more concentrated luminosity. Faint and diffuse light extends from the central region, tracing the galaxy's disk. There appears to be evidence of a slight warp or asymmetry in the disk's outer regions. The disk presents a complex structure with subtle features such as minor disturbances. The light from the galaxy is relatively faint. The color profile suggests the presence of both older stellar populations (redder light) in the bulge and disk, and hints of younger, bluer populations within the outer regions of the disk, potentially indicating on-going star formation.
