The galaxy presents as a centrally concentrated system with a bright, relatively smooth core, likely an elliptical galaxy. The main body exhibits a slight elongation. The central region displays a yellowish hue, potentially indicating an older stellar population. Fainter, bluish regions are present in the outer disk, perhaps indicative of younger stars and some ongoing star formation, although this is relatively subdued. A potential tidal feature is visible in the upper left quadrant, suggesting a past or ongoing interaction with another galaxy. The overall morphology suggests a relatively evolved system, with the possibility of recent or ongoing minor merger activity.
