The galaxy appears as a centrally concentrated object with a relatively smooth morphology. There is a slight asymmetry or possible faint arm-like structure discernible, but overall, it presents as a fairly regular, elliptical-like shape. The core exhibits a brighter intensity, suggesting a possible bulge. There is no obvious dust lane or prominent spiral structure, and it seems relatively isolated, showing no signs of major interaction or ongoing merger activity. Its round shape is most prominent. The galaxy's overall color appears slightly reddish, suggesting a population of older stars and relatively little ongoing star formation. There might be some indication of minor disturbances in its structure.
