This galaxy appears to be a disk galaxy viewed edge-on. A prominent bulge is observed, with a shape that seems more rounded than boxy. There is evidence of a disk structure. The disk appears relatively smooth and lacks distinct features. The central bulge exhibits a reddish hue, possibly indicating an older stellar population and/or dust obscuration. The outer regions of the disk show some bluer color, suggestive of some star formation, though not at a high rate. No major disturbances or signs of mergers with other galaxies are readily apparent, although subtle asymmetries may indicate minor tidal interactions. Overall, the galaxy presents a fairly regular morphology, consistent with a galaxy that has not undergone recent major disruptive events.
