The galaxy appears to be a relatively smooth, elliptical galaxy. The light distribution suggests a centrally concentrated spheroid.  It exhibits a slight elongation, appearing more cigar-shaped than perfectly round. There's a subtle color gradient, with the central region appearing more yellowish, possibly indicating an older stellar population or a higher concentration of dust attenuating shorter wavelengths. No distinct spiral arm structure or significant dust lanes are discernible.  There are no signs of any ongoing major merger events. The galaxy shows no evidence of tidal tails or other strong gravitational disturbances, and the overall impression is one of a galaxy that has reached a dynamically relaxed state.
