The galaxy presents as a slightly elongated, centrally concentrated object. The light distribution appears relatively smooth, with a hint of a flattened, disk-like structure but could also just be an indication of a faint ring system. A fraction of light suggests possible disturbances or tidal features, indicating potential interactions with another galaxy, there is the potential for it to be experiencing a merger. The color index shows a shift towards the redder end, it is unlikely to be currently forming many stars. The central region appears brighter, possibly indicating the presence of an active galactic nucleus or a high concentration of older stars. A subtle color gradient is observed, with the inner regions appearing slightly redder than the outer regions. The galaxy exhibits a subtle elongated shape, the galaxy appears to be neither perfectly spherical nor highly flattened. Overall, it presents as a potentially isolated galaxy with a dominant smooth component and a faint disklike component and shows the possibility of having experienced recent interaction. 
