The galaxy presents as a highly elongated, edge-on spiral. A distinct central bulge is visible, exhibiting a reddish hue that may indicate an older stellar population. The disk appears relatively thin and exhibits a blueish color suggesting the presence of younger, hotter stars and ongoing star formation. The galaxy displays a smooth, symmetrical profile along its major axis, with no signs of major tidal disturbances or ongoing mergers. The outer edges of the disk appear somewhat diffuse, potentially indicating a gradual decline in stellar density. Overall, the galaxy presents as a well-defined, undisturbed edge-on spiral system.
