The observed galaxy presents a relatively smooth, elliptical morphology. The central bulge exhibits a concentrated luminosity, appearing bright and slightly yellow-orange. The light gradually diffuses outwards, indicating a lessening density of stars. The galaxy's overall shape is somewhat elongated, not perfectly spherical, with a relatively large semi-major axis compared to its semi-minor axis. There is no clear evidence of spiral arm structures or significant dust lanes. Minimal signs of tidal distortions or ongoing major mergers are apparent, though a potential minor disturbance cannot be entirely ruled out based on this image alone. The overall color suggests an older stellar population, with fewer young, massive stars contributing to the luminosity.
