This galaxy exhibits a roughly elliptical morphology, appearing somewhat elongated. A bright central bulge is prominent, characterized by a yellowish-white hue, suggesting an older stellar population. Fainter, more diffuse light extends outwards from the bulge, forming a halo or disk-like structure with a reddish tinge. There is subtle evidence of disturbed morphology, potentially indicating an ongoing or recent interaction. The galaxy presents no clearly defined spiral arms. The overall color suggests a relatively low star formation rate within the observed region.
