The galaxy appears to be a relatively smooth, elliptical system. It exhibits a concentrated central bulge that dominates the overall morphology. The light distribution is fairly uniform, without prominent spiral arms or distinct features. There is a slight color gradient, with the central region appearing more yellowish-orange, suggesting an older stellar population. Fainter, more diffuse blue light is visible in the outer regions, potentially indicating some ongoing, albeit low-level, star formation. The galaxy exhibits a generally round shape, with no obvious signs of significant tidal disturbances or ongoing mergers. 
