The galaxy presents a generally smooth appearance with a bright central bulge. The light distribution suggests an elliptical morphology, although a slight disk component may be present. The galaxy does not show any signs of major disturbances or merging events. It has a concentrated light profile indicative of a relatively old stellar population, with bluer wavelengths in the center compared to the outer regions. The isophotes of the galaxy appear to be more rounded than elongated. No prominent spiral arm structures or dust lanes are clearly visible. The overall color of the galaxy is indicative of moderate star formation activity.
