The galaxy presents as an elliptical or lenticular type, appearing largely smooth with a noticeable lack of spiral arm structures or prominent dust lanes. Its overall morphology leans towards being rounded, with a moderate ellipticity. The galaxy exhibits a color gradient, transitioning from a bluer hue in the central region to a redder, yellower tone in the outer regions. This color shift likely indicates a centrally concentrated population of younger, hotter stars, giving way to a more dominant population of older, cooler stars in the galactic halo. There are subtle indications of possible minor tidal disturbances or interactions, which appear as faint, wispy extensions or irregularities around the main galactic body. The overall structure suggests a galaxy that has largely completed the major merging events in its past.
