The galaxy appears to be a relatively smooth, elliptical-like system. It exhibits a concentrated central bulge that is bright, transitioning into a fainter, more diffuse halo. The light distribution is mostly even throughout, which could indicate an older stellar population with minimal recent star formation. There may be a slight hint of disk structure, but it is not very prominent. The galaxy's shape is close to circular, without any significant tidal distortions or evidence of ongoing mergers. There are hints of dust extinction in the outer regions of the galaxy. The system lacks any strong spiral arm structure or distinct features, suggesting a lack of significant ongoing star formation. The color of the light is weighted slightly toward redder wavelengths, which is also consistent with an older stellar population. 
