The galaxy presents an elliptical morphology, appearing largely smooth and spheroidal in shape. It displays a concentrated central bulge that emits primarily in the yellow-red wavelengths, indicating a population of older, evolved stars. The color suggests minimal ongoing star formation within the bulge. A faint halo of light extends outwards, fading into the background sky. There may be some minor distortions or asymmetry in the galaxy's outer regions. This suggests a possible interaction or recent minor merger event, though the dominant appearance is that of a relaxed system. The galaxy is likely a relatively massive system, and the stellar population indicates it is undergoing slow or little star formation.
