The galaxy appears as a roughly elliptical structure, with a bright, concentrated central bulge. The overall color profile suggests a population of older stars, biased towards redder wavelengths, most prominently in the bulge. Fainter, bluer regions extend outwards from the central bulge, hinting at the presence of a disk component and potentially younger stellar populations. The galaxy appears relatively smooth with some subtle irregularities or disturbances in the outer disk, which may be indicative of minor interactions or internal dynamics. There are no obvious signs of significant ongoing star formation, but the bluer regions indicate there is some present. The galaxy’s light is elongated along one axis, suggesting it may be an elliptical galaxy with some residual disk-like structure or a spiral galaxy seen at a high inclination.
