The galaxy presents a generally smooth, elliptical morphology. The light is concentrated in the center, with the luminosity appearing to gradually decrease outwards. The shape is neither perfectly round nor highly elongated, appearing as an intermediate, slightly oval form. There is a central core region with a blue-ish hue, potentially indicative of recent or ongoing star formation. Little to no spiral arm structure is visible. No significant disturbances such as tidal tails or strong asymmetries are apparent, suggesting that it is not undergoing any major merging activity. It appears to be a relatively isolated galaxy, undisturbed by external gravitational forces from nearby galaxies.
