The galaxy presents as a relatively smooth, elliptical structure. There is a concentrated, bright central bulge exhibiting a yellow-orange hue, suggesting an older stellar population and possible dust obscuration. Moving outward from the center, the galaxy appears to fade into a less distinct halo or envelope with a slightly bluer tint, possibly indicating some ongoing, albeit subdued, star formation in the outer regions. The overall shape leans towards being somewhat elongated, but not severely cigar-shaped. There is no readily apparent evidence of strong tidal interactions or major disturbances in its morphology, implying it is a relatively undisturbed system. The structure is generally smooth and well-defined indicating either an elliptical galaxy or a spiral galaxy viewed at a significant inclination.
