This galaxy appears to be an elliptical galaxy with some disk-like features. It exhibits a smooth, diffuse structure, with a brighter central bulge. The galaxy appears elongated, with an axial ratio suggesting it is not perfectly spherical. There is also a hint of spiral arm structure. The color gradient suggests that the core of this galaxy is populated by older stars, as indicated by the redder hue, while the outer regions have hints of bluer regions that indicate a more recent star formation rate. There is no evidence of a major merger. There is no obvious dust lane or other clear signs of significant obscuration.
