The galaxy appears to be elliptical or lenticular, exhibiting a generally smooth morphology with a high degree of central concentration. The light profile suggests a centrally dominant bulge component, as evidenced by the concentration of yellow light in the central region. There are no clearly resolved spiral arms or bar structures visible. The galaxy has a well-defined, elliptical shape with a high degree of roundness. There is no apparent major disturbance or merger activity evident in the image. The galaxy exhibits a moderate amount of star formation activity, likely in the central region of the galaxy.
