The observed galaxy presents a notable disk-like structure, viewed at an intermediate angle. A prominent central bulge exhibits a concentrated luminosity profile, transitioning smoothly into a fainter, more diffuse disk. Within the disk, there is tentative evidence of spiral arm structures, though these are not sharply defined. The overall color of the galaxy is yellowish-white, suggesting a relatively mature stellar population. There is no obvious indication of ongoing major mergers or tidal disturbances.
