The galaxy presents as a lenticular or possibly a spiral galaxy viewed nearly edge-on. A central bulge is prominent, appearing yellowish-white, suggesting a population of older stars. The disk is visible, exhibiting a slightly bluer hue compared to the bulge. This color variation potentially indicates the presence of ongoing, albeit perhaps limited, star formation within the disk component. The galaxy's overall structure appears relatively undisturbed, showing no major signs of ongoing or recent merger activity. Some minor asymmetry might be present but is difficult to confirm due to resolution limits.
