This galaxy presents as an edge-on spiral, exhibiting a prominent, elongated disk structure. The disk appears relatively smooth and featureless. There is evidence for a classical bulge that dominates the galaxy's central region. The bulge appears symmetrical, potentially harboring a supermassive black hole, though direct observation is limited by the edge-on orientation. No distinct spiral arm structure is discernible from this viewing angle. The lack of significant dust lanes suggests a possible lack of active star formation in the disk. The galaxy appears to show hints of merging activity, possibly a small companion in the vicinity. The luminosity profile seems consistent with an older stellar population, displaying light shifted towards the redder end of the spectrum.
