The galaxy appears to be a spiral galaxy viewed nearly edge-on. A prominent central bulge is visible, exhibiting a yellowish-orange hue, likely indicating an older stellar population. Fainter, bluish light emanates from the galactic disk surrounding the bulge, suggesting the presence of younger, hotter stars. The disk appears relatively smooth, with little evidence of distinct spiral arms. The galaxy appears to be relatively undisturbed with no major mergers. There might be minor disturbances, such as tidal tails or asymmetric features, but they are not clearly observable.
