This galaxy presents as a lenticular or possibly a spiral galaxy viewed edge-on. A prominent central bulge is observed, exhibiting a yellowish-white hue, indicative of an older stellar population. This bulge transitions smoothly into a fainter, bluish-white disk. The disk appears relatively thin and elongated, with the bluer color suggesting the presence of younger, hotter stars and ongoing star formation. The dust lanes are not highly defined but may be present, further suggesting a possible spiral morphology. There appears to be some minor disturbance visible, in the form of a subtle warping or asymmetry to the galaxy's disk, possibly suggesting a past or ongoing interaction with another galaxy. There appears to be no clear evidence of a strong, ongoing merger. Overall, this galaxy appears as a relatively evolved system with a mix of stellar populations and a disk-like structure.
