The galaxy presents as a relatively smooth, centrally concentrated object. Its shape is generally round. There is no strong evidence of spiral arms or a distinct disk component based on the limited resolution. The galaxy exhibits a color gradient, with a slightly bluer hue toward the core. This bluer color may indicate a region of ongoing star formation, albeit at a moderate rate. There is no visual evidence of any major mergers or tidal disturbances affecting its structure, and the galaxy appears relatively isolated.
