The galaxy presents as a lenticular or possibly a spiral galaxy viewed edge-on. A prominent dust lane bisects the galaxy along its major axis, obscuring light from the central bulge. This obscuration is most apparent toward the galaxy's center, suggesting a relatively high concentration of dust within the galactic disk. The bulge appears to be mildly boxy, or peanut shaped. Little to no arm structure is visible, but there may be minor irregularities along the disk that could be attributed to star formation. The galaxy appears relatively undisturbed, with no major signs of recent mergers or tidal interactions. The galaxy exhibits a redder hue overall, indicative of an older stellar population and potentially lower levels of ongoing star formation. The estimated physical size based on half-light radius is approximately 7 kpc.
