This galaxy exhibits a generally elliptical morphology. There is a central, concentrated bulge that appears yellowish. The light from this region is relatively smooth and consistent, suggesting an older stellar population. Extending outward from the core, there is a fainter, diffuse halo of light with a bluish tinge. The gradient from the core to the outer regions is gradual, indicating that the stellar density decreases smoothly with increasing radius. The overall shape suggests a system that is more elongated than circular, with a cigar-like appearance. There is no clear indication of strong spiral arm structures or active galactic nuclei. There is a very slight hint of minor disturbances or irregularities in the outer halo, but overall the galaxy appears to be a relatively undisturbed, evolved system.
