The galaxy exhibits a distinct disk morphology, viewed nearly edge-on from our line of sight. This perspective obscures any potential spiral arm structure. The central bulge appears elongated and somewhat boxy, but is difficult to resolve due to the viewing angle. There is a slight asymmetry to the galaxy's shape. The color distribution suggests a higher concentration of older stellar populations, with a dominant orange-red hue throughout the disk. Evidence of dust lanes are subtle, although not non-existent in certain areas of the disk. There are no obvious signs of a major merger or significant tidal disturbances, though minor disturbances cannot be ruled out. The galaxy appears to be moderately luminous.
