The galaxy presents as a lenticular system viewed edge-on. It exhibits a prominent central bulge, appearing relatively smooth and spheroidal, with a concentration of light intensity at its core. The galactic disk appears as a faint, extended structure bisecting the bulge, with an apparent lack of distinct spiral arm features. The disk is relatively thin, and there's some indication of dust lane absorption along the equatorial plane, attenuating the light and lending a slightly darker hue compared to the rest of the galaxy. The galaxy appears largely undisturbed, lacking any obvious signs of recent major merger events or tidal disruptions. The overall color suggests a population dominated by older stars, with relatively low levels of on-going star formation.
