The galaxy presents a predominantly smooth morphology. It exhibits a centrally concentrated light profile, suggesting a significant bulge component. The shape appears to be mostly round. There is some visual evidence of faint, diffuse outer regions extending beyond the bright central bulge. Color gradients indicate a bluer hue in the outer regions compared to the yellower core. There is no obvious dust lane or spiral arm structure visible. The overall impression is that of a relatively quiescent system, with no major signs of ongoing merger activity or significant star formation.
