This galaxy exhibits a generally smooth morphology. The central region presents a high concentration of light, appearing bright and somewhat yellowish, suggesting an older stellar population. Surrounding the core is a more diffuse, bluish halo. This could be indicative of more recent star formation within the outer regions. There is a slight asymmetry to the halo, hinting at a possible minor interaction or disturbance but no obvious signs of a major merger event. The overall shape is roughly elliptical.
