The galaxy appears as a diffuse, luminous object with an elliptical morphology. It exhibits a smooth texture overall, with the majority of its light concentrated in a central bulge. The galaxy displays a color gradient, shifting from a yellow/orange hue in the central region to a somewhat redder tone in its outer fringes. There is a secondary concentration of light below the main body which may indicate it is a merging galaxy. No distinct spiral arm structures or dust lanes are apparent. The galaxy's outer edges gradually fade into the background, with a relatively concentrated core, suggesting a lack of active star formation in the disk. The smoothness and color profile suggest an older stellar population dominates the galaxy's composition. There may be a minor tidal disturbance occurring.
