This galaxy appears to be an edge-on spiral galaxy, exhibiting a prominent central bulge and a flattened disk. The bulge displays a smooth, concentrated luminosity profile with a yellowish-white hue suggesting an older stellar population. A small number of dust lanes might exist within the galaxy, although low image quality makes this difficult to confirm. The lack of defined spiral arms and its generally smooth morphology suggest a relatively quiescent star formation rate. The elongation of the galaxy indicates a high inclination angle, likely very close to 90 degrees relative to our line of sight. Its overall structure is undisturbed, showing no obvious signs of recent major mergers or interactions. The absence of bright HII regions or intense blue star formation regions supports the interpretation of a galaxy with a relatively low specific star formation rate.
