The galaxy presents as an elliptical-like morphology, with a high degree of central concentration and a relatively smooth, diffuse light profile. The object displays a moderate degree of roundness. There is little evidence of spiral arm structure or a prominent disk. No obvious tidal features or signs of ongoing major mergers are apparent, though a minor disturbance cannot be ruled out. The galaxy exhibits a reddish hue, suggesting an older stellar population and potentially lower ongoing star formation activity. 
