The galaxy presents as a moderately bright, somewhat elliptical object. The central region appears smooth and displays a concentration of light, suggesting the presence of a bulge. A fainter, more diffuse disk-like structure surrounds the core. This outer region appears slightly asymmetric, with indications of possible disturbances or faint spiral arm segments. The color distribution suggests a population of relatively old stars with a hint of younger, star-forming regions due to a blueish presence in the outer regions. There is no obvious signature of a major merger event, though minor disturbances could be present.
