The galaxy appears as a relatively smooth, centrally concentrated object with a slightly elliptical morphology. The core exhibits a bright, yellowish-white hue, suggesting an older stellar population. Diffuse, bluish extensions emanate from the central region, hinting at possible star formation. These extensions do not show well-defined spiral arm structures. There is no obvious evidence of a major ongoing merger, though a slight asymmetry and some faint wisps indicate a possibility of a minor interaction. The galaxy appears moderately massive and demonstrates low star formation activity. Overall, the galaxy seems to be a relatively passive system in its evolutionary stage.
