The galaxy appears to be a relatively smooth, elliptical type. It exhibits a concentrated central bulge that transitions into a more diffuse halo. There is little to no apparent spiral arm structure, and the galaxy lacks strong features indicative of active star formation. The color gradient suggests that the central region is dominated by an older stellar population, while the outer regions may contain younger stars. Overall, the galaxy presents a fairly undisturbed morphology with minimal signs of recent mergers or tidal interactions. The shape of the galaxy is round.
