The galaxy presents as an edge-on spiral, exhibiting a clear disk structure viewed at a high inclination. The central bulge is prominent and appears to be largely spherical. The dust lane is not distinctly visible, although there are indications of some obscuration along the midplane of the disk. The galaxy has a noticeable color gradient, with the bulge appearing yellower. Based on the color, stellar population, and morphology, this galaxy likely has a relatively high mass and a low specific star formation rate. I do not see any evidence of tidal tails or shell structures, indicating that it likely has not experienced a recent major merger event.
