The galaxy presents as an elongated, edge-on spiral. A central bulge is discernible, exhibiting a yellowish-orange hue, possibly indicating an older stellar population. The disk appears relatively thin and smooth, lacking prominent spiral arm structure. There is little evidence of significant dust lanes or active star formation regions from this vantage point. The overall morphology suggests a galaxy that may have exhausted much of its gas reservoir, and with a likely lower recent star formation rate. The disk shows a faint blue tinge toward the outer edges, hinting at the presence of some younger, hotter stars, though not in quantities to make the galaxy appear distinctly blue. There is no clear evidence of any major ongoing merger activity or significant tidal disturbances. Subtle signs may indicate minor perturbations, but these are not pronounced.
