The galaxy presents as a somewhat elongated, lenticular or possibly spiral structure viewed at a significant angle. The central bulge appears bright and yellowish-white, suggesting an older stellar population. Proceeding outward from the bulge is a fainter, bluer disk, indicating the presence of younger, hotter stars and possibly some ongoing star formation, though limited. The disk appears relatively smooth, lacking prominent spiral arm structure. There is a slight asymmetry or minor irregularity in the morphology, hinting at a potential interaction or recent merger event. The overall appearance suggests a relatively massive galaxy.
