The galaxy presents as a centrally concentrated object with a moderately elongated shape. The core region exhibits a yellow-white hue, suggesting a population of older stars. A subtle redder gradient is observed extending outwards from the core, potentially indicating an aging stellar population or dust obscuration. The outer regions appear relatively smooth, with little evidence of distinct spiral arms or prominent star-forming regions. There's a very slight asymmetry in the galaxy's overall shape; a faint extension appears at one end, barely noticeable. This could be an indication of a tidal interaction or minor disturbance, but it could also be an artifact. The morphology is generally smooth, with the galaxy appearing relatively undisturbed and quiescent in its current state. Based on its color and morphology, it is likely a galaxy that is not highly active in star formation.
