This galaxy presents as an edge-on spiral, exhibiting a prominent, elongated disk structure. The central bulge is notably bright and appears to be a yellow-red hue, possibly indicative of an older stellar population. The disk shows faint blue regions along the edge. The galaxy's disk appears relatively smooth. Dust lanes are not readily apparent, but this could be due to the resolution of the image or a more face-on alignment of the dust within the disk. The overall appearance suggests a relatively high mass galaxy, with ongoing, moderate levels of star formation, particularly concentrated within the disk component. There are no signs of significant disturbances or tidal features, suggesting this galaxy has not undergone any major mergers recently.
