This galaxy exhibits a morphology that is neither definitively smooth nor distinctly featured, presenting a blend of characteristics. The overall form appears to be somewhat elliptical, with a moderate degree of roundness rather than being highly elongated. 

A central bulge is evident, characterized by a yellowish-white hue, suggesting an older stellar population. Surrounding this bulge is a fainter disk or halo component, displaying a slightly bluer tint, implying the presence of younger stars and possibly some ongoing star formation. There might be some disturbances. However, the galaxy shows no strong evidence of a major merger event, though minor disturbances cannot be ruled out.

The galaxy appears to be a relatively massive system with signs of moderate star formation.
