The galaxy presents as a relatively smooth, elliptical-like structure. The central bulge exhibits a concentrated, bright yellowish hue, suggesting an older stellar population dominated by redder stars. Moving outwards from the core, the light gradually fades into a softer, whitish halo, indicating a more dispersed distribution of stars. There is a slight elongation along one axis, giving it a somewhat cigar-shaped appearance, though it is mostly rounded. There is a very subtle hint of a disk structure. No prominent spiral arms or dust lanes are visible, suggesting a lack of ongoing, large-scale star formation, although a small amount of star formation may be occurring. The galaxy appears relatively undisturbed, showing no signs of major mergers or tidal interactions.
