The galaxy appears as a relatively smooth, centrally concentrated object. It exhibits a slightly elongated, possibly elliptical shape, with an apparent lack of prominent spiral arms or a well-defined disk structure. The color distribution indicates a relatively uniform stellar population, primarily exhibiting yellowish hues throughout the galaxy's main body, hinting at an older, more evolved stellar population with ongoing star formation. There is a hint of bluer regions scattered within the galactic structure, possibly indicating regions of more recent star formation. There is a slight asymmetry to the galaxy's light distribution. There may be signs of minor disturbances or tidal features. The morphology suggests a system that may have undergone recent interactions or mergers.
