The galaxy presents as a largely featureless, elliptical morphology. It appears smooth and relatively round, with a concentrated central bulge that emits strongly in the yellow-orange wavelengths. The color profile suggests an older stellar population, with a lower rate of star formation compared to actively star-forming spiral galaxies. The overall color is dominated by redder wavelengths with some emission in the green-yellow wavelengths, indicative of aging stars. There is no obvious presence of spiral arms or a prominent disk structure in this image. Any sign of recent merging events or other irregularities appears minimal. Overall, it is a typical, somewhat small elliptical galaxy, likely with a significant red shift.
