The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge that appears yellowish in color, suggesting an older stellar population. The outer regions exhibit a slightly bluer hue, possibly indicating the presence of younger stars or some ongoing star formation, though the overall rate is likely low. The galaxy lacks any prominent spiral arms or distinct disk-like features. There may be minor distortions or slight asymmetries in its shape. The galaxy doesn't seem to be undergoing any major merging events. Overall, it appears to be a mature, relatively quiescent galaxy with a substantial mass.
