The galaxy appears to be an elliptical galaxy. It exhibits a smooth, centrally concentrated morphology, with a high degree of radial symmetry. The galaxy's light profile suggests a relatively homogenous stellar population and dust content. The core exhibits a yellowish hue, likely indicating an older stellar population. There is little evidence of spiral arms, active star formation regions, or significant dust lanes. The isophotes appear mostly regular with no significant tidal features or signs of ongoing major mergers, suggesting it has largely completed its formation. A slight deviation from perfect roundness is perceptible. The galaxy is relatively massive with moderate ongoing star formation.
