The galaxy presents as a relatively smooth, disk-like structure oriented nearly edge-on from our perspective. The central bulge is noticeable and appears moderately bright and concentrated, possibly indicating an older stellar population. Faint, diffuse arms extend outwards from the bulge, exhibiting a slightly mottled texture that might suggest some star formation. There's a hint of blueish color within the disk, which could be attributed to the presence of younger, hotter stars. Overall, the galaxy's morphology suggests an intermediate type between a pure elliptical and a spiral, possibly a lenticular galaxy experiencing minor disturbances.
