This galaxy appears to be a relatively smooth, elliptical galaxy. It exhibits a concentrated central bulge, with a gradual decrease in luminosity moving outward. The core displays a yellowish-white hue, suggesting an older stellar population, while the outer regions have a slightly bluer tint, implying the presence of some younger stars, and possibly some ongoing star formation. There is no obvious disk structure or spiral arms visible. The overall morphology indicates a lack of significant disturbances. The galaxy is roughly circular in appearance. The galaxy appears to be quite massive.
