The galaxy presents as a relatively smooth, elliptical-like structure with a bright central bulge. It exhibits a dominant, almost spherical shape, with a slightly elongated appearance along one axis. The color profile suggests a population of older stars, particularly concentrated in the core. Fainter, diffuse bluer emissions are visible surrounding the central region, indicating some presence of younger stars or ionized gas, although the overall star formation rate appears low. There is no obvious evidence of spiral arms or significant dust lanes. The overall morphology is largely undisturbed. There are no apparent signs of major merger events or tidal disturbances.
