The galaxy presents as a somewhat elongated structure, suggestive of an elliptical or possibly a late-type spiral galaxy viewed edge-on. The central region exhibits a concentrated luminosity, transitioning smoothly into a fainter, more diffuse outer halo. There's a slight asymmetry in the isophotes, hinting at possible tidal interactions or internal disturbances, although no distinct merger features are readily apparent. The color gradient suggests an older stellar population dominating the central bulge, while the outer regions might contain a small population of younger, bluer stars. Overall, the galaxy appears relatively undisturbed, exhibiting a well-defined, coherent structure.
