The galaxy presents as a largely smooth, centrally concentrated object, likely an elliptical galaxy. A subtle color gradient is visible, shifting from a bluer hue in the outer regions to a slightly redder core. The central region exhibits higher luminosity, indicative of a dense stellar population. The galaxy appears relatively isolated, without any obvious signs of ongoing major mergers or tidal distortions, though minor disturbances cannot be ruled out at this resolution. The overall shape is roughly circular with the absence of any prominent disk features or spiral arms.
