The galaxy presents as a relatively smooth, elliptical or lenticular type, elongated in shape with a high axis ratio. The light distribution appears centrally concentrated with a diffuse, fading profile towards the edges. A subtle bluish hue is observed within the central region, suggesting recent or ongoing star formation, albeit at a low rate. There is no obvious presence of spiral arms or a prominent disk. The galaxy exhibits no major signs of tidal disturbances or ongoing mergers, though some minor asymmetries or distortions are not entirely ruled out. Overall, the galaxy appears to be a relatively isolated and quiescent system.
