The galaxy presents as a relatively smooth, elliptical-like object with a concentrated central bulge. The core region displays a yellowish hue, suggesting an older stellar population. Fainter, diffuse emissions extend outwards from the core, exhibiting a slight greenish tint in some areas, potentially indicating some level of ongoing star formation, but with a dominant population of older stars overall. The galaxy appears to have a fairly regular morphology, with no obvious signs of major disturbances or tidal features indicative of recent mergers, though minor irregularities or subtle disturbances cannot be ruled out at this resolution. The galaxy has a slightly elliptical shape, and its morphology suggests a system that is nearing the end of its life cycle.
