The galaxy presents a largely smooth, elliptical morphology, appearing relatively featureless at this resolution. The light is concentrated toward the center, exhibiting a bright, well-defined nucleus. Moving outward from the core, the light gradually diffuses, indicating a decreasing stellar density with radial distance. The galaxy exhibits a moderate ellipticity, deviating somewhat from a perfectly circular shape. Color gradients appear subtle; the central region presents a slightly yellower hue, potentially indicating an older stellar population, while the outer regions exhibit a marginally bluer tinge, possibly indicating the presence of younger stars, though at very low numbers. No spiral arm structures or significant dust lanes are discernible. There is a secondary light source, suggestive of either tidal interactions or perhaps a background object that isn't interacting with the main galaxy.
