The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a central concentration of luminosity, suggesting a bulge component. There is little evidence of significant star formation in the visible bands, as indicated by the lack of prominent blue regions. The galaxy does not appear to be undergoing any major merger events, though a slight asymmetry in the light distribution might suggest minor past interactions or disturbances. Overall, the galaxy appears to be a relatively evolved system, consistent with a redder color profile. The shape appears more round than cigar-shaped. 
