The galaxy exhibits a generally elliptical morphology, appearing relatively smooth with a high degree of central concentration. The light distribution suggests a prominent bulge component, gradually decreasing in intensity outwards from the core. The galaxy is observed at an inclination angle that is neither face-on nor edge-on, but rather appears to be at a slight angle. There is no obvious presence of spiral arm structures or distinct dust lanes. The color is consistent with an older stellar population, the light is a yellow/white hue indicating a lack of recent star formation. There is no evidence of active galactic nuclei activity or interaction with other galaxies.
