The galaxy presents a generally smooth, elliptical morphology. The light profile appears centrally concentrated, with a gradual decline in intensity outwards. The galaxy exhibits a subtle elongation along one axis but does not display any distinct spiral arm structures or prominent dust lanes. Its color is overall redder, suggesting an older stellar population. There is no evidence of active galactic nuclei activity or ongoing star formation. There might be faint tidal features that suggest past interactions, but more detailed images are needed to confirm. The galaxy is most likely an elliptical galaxy, with minimal active star formation.
