The galaxy presents as an elongated, disk-shaped structure oriented approximately edge-on to our line of sight. A distinct central bulge is not readily apparent; instead, a somewhat uniform brightness distribution characterizes the central region.

The galaxy exhibits a color gradient, transitioning from bluer hues at one end to redder hues at the opposite end. The bluer end may indicate a region of ongoing star formation, while the redder end may denote an older stellar population or regions of dust obscuration.

The morphology appears to be that of a relatively undisturbed spiral galaxy. No obvious signs of tidal tails, asymmetries, or other disturbances indicative of recent mergers are visible. The galaxy exhibits a moderate surface brightness. There is faint, diffuse emission extending beyond the main body of the galaxy, possibly representing a faint halo or extended disk.
