The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a moderate degree of ellipticity, appearing mostly rounded but slightly elongated. No obvious spiral arm structures or a prominent disk are discernible in this image. The galaxy's light profile appears to decrease fairly smoothly from the center outward, and does not show signs of any recent major merger activity, but appears to have experienced minor disturbances in the past. The light from the galaxy is a mix of colors, with a prominent red component and some contribution from the green and blue filters. Given the estimated luminosity and color, the galaxy probably harbors a supermassive black hole. It shows a modest amount of star formation activity. The overall morphology suggests this is likely a galaxy toward the red sequence.
