The galaxy exhibits a smooth, elliptical morphology. It appears centrally concentrated with a bright, diffuse core that fades gradually into the outer regions. There is a slight elongation, indicating a possible oblate spheroidal shape, although it is mostly rounded. The galaxy's color gradient suggests an aging stellar population, with a yellowish hue dominating the central bulge. There is no apparent disk structure, spiral arms, or signs of recent major merger activity within this observed field. Slight color variations may indicate differential dust absorption or patches of differing stellar populations, though the lack of distinct features suggests a relatively quiescent, evolved galaxy.
