The galaxy presents as a relatively smooth, elliptical or lenticular structure. It appears largely featureless, with a highly concentrated central bulge and a diffuse halo. There is minimal evidence of spiral arms or significant dust lanes. The galaxy exhibits a fairly uniform color gradient, with a slightly bluer hue at the center gradually fading to redder tones in the outer regions. This color distribution may be indicative of ongoing star formation in the core, or it may simply be a result of dust extinction in the outer regions. Overall, the galaxy seems to be well-evolved, with no obvious signs of recent major mergers or tidal disturbances. 
