The galaxy presents as a single, relatively smooth object with a concentrated central bulge. The color profile suggests an older stellar population, leaning towards a redder hue overall. There is minimal evidence of spiral arms or significant dust lanes. The galaxy appears elliptical in shape. Given the redshift, the light emitted from the galaxy is shifted towards the red end of the spectrum, indicating that the galaxy is receding from our location due to the expansion of the universe. We observe a low rate of star formation.
