The galaxy presents a largely smooth, elliptical morphology. There is little indication of spiral arm structure or significant dust lanes. The galaxy core appears highly concentrated, with light intensity diminishing gradually towards the periphery. Color gradients within the galaxy are subtle, with a slightly redder hue in the central regions compared to the outer halo. There is no strong evidence of ongoing merger activity or tidal distortions. Given its estimated size, high degree of central concentration and smooth light profile, this galaxy is likely a fairly massive system, exhibiting characteristics of a mature elliptical galaxy. There are no discernible HII regions indicating active star formation. The overall visual impression suggests a quiescent stellar population with a minimal contribution from young, massive stars.
