The galaxy appears as a relatively smooth, elliptical-like structure. Its light is concentrated towards the center with a gradual decrease in intensity towards the edges. The core region is a yellowish-orange hue, suggesting an older stellar population. There are no prominent spiral arms or distinct features typically associated with disk galaxies. The overall color profile indicates a redder galaxy, which often correlates with reduced star formation activity. There is no visual evidence of any major ongoing merger events or significant tidal disturbances impacting the galaxy's structure. The object exhibits a moderate level of roundness with a slight deviation from a perfectly circular shape.
