This galaxy presents as a spindle or cigar-shaped morphology, likely an edge-on spiral or lenticular galaxy. The central bulge appears relatively prominent, exhibiting a reddish-orange hue, suggesting a population of older, redder stars. Moving outwards from the bulge, a flattened disk is observed, displaying a bluer color, indicative of younger, hotter stars and potential ongoing star formation. The overall appearance is relatively smooth, with only slight hints of possible dust lanes or substructure within the disk. There seems to be minimal evidence of significant tidal disturbances or interactions with other galaxies, suggesting a relatively isolated system.
