The galaxy exhibits a roughly elliptical morphology, appearing somewhat elongated. The central bulge is bright and concentrated, displaying a yellowish-white hue, suggesting an older stellar population. Surrounding the central region, there's a fainter, more diffuse halo with a bluish tint. This color variation indicates the presence of some ongoing or recent star formation in the outer regions, although less intense than what would be observed in a spiral galaxy with prominent arms. There's no clear evidence of spiral arm structures, but the outer disk appears to be somewhat irregular, suggesting a mild disturbance or interaction in its past. Overall, the galaxy presents characteristics of an intermediate type, potentially between a pure elliptical and a spiral galaxy.
