The galaxy presents as an elliptical morphology, with a high degree of radial symmetry. The light distribution appears centrally concentrated, with brightness decreasing smoothly outward from the nucleus. The core exhibits a yellowish hue, suggesting an older stellar population. Faint, diffuse blue light is observed in the surrounding region, potentially indicative of a small amount of more recent star formation. There is no clear evidence of spiral arms or a bar structure. No signs of tidal tails or strong distortions are visible, which suggests this galaxy is relaxed, with no recent major merger events, though possibly minor disturbances. The smooth light distribution and the dominance of redder colors point towards a galaxy with evolved stellar populations and a low star formation rate.
