This galaxy presents as a relatively smooth, elliptical-type object with a noticeable central bulge. The light distribution is concentrated towards the center, exhibiting a radial gradient in surface brightness, with the core appearing significantly brighter than the outer regions. The galaxy has a generally round shape with a slight elongation. There is a subtle color gradient apparent, trending towards slightly redder hues in the central region, possibly indicating an older stellar population there. No prominent spiral arms or dust lanes are visible. The overall appearance is consistent with a mature galaxy that has likely undergone significant internal relaxation and evolution. There is little evidence of recent or ongoing major mergers, however there may be some signs of minor disturbance. 
