The object presents as a lenticular galaxy, viewed nearly edge-on. It exhibits a smooth, elongated morphology, with a discernible bulge dominating the central region. The bulge displays a yellowish hue, likely indicating an older stellar population. Faint disk features can be observed extending outwards from the bulge, subtly tinged with bluish colors, suggestive of the presence of some younger stars or ongoing star formation. There appear to be no signs of major disturbances or merging events, with a generally undisturbed structure. The galaxy appears to have a substantial stellar mass and a moderate star formation rate.
