The galaxy presents as a smooth, elliptical morphology, exhibiting a largely featureless structure. Its light profile is concentrated centrally, fading gradually towards the outer regions, indicating an absence of prominent spiral arms or significant star-forming regions. The primary color appears to be a yellow-white hue, which may suggest an older stellar population that primarily contains Population II stars. There is little evidence of dust lanes or ongoing merger activity that would disrupt the galaxy's smooth appearance. The overall shape is nearly circular, showing a slight deviation from perfect sphericity. Some possible minor tidal disturbances may be present, but would require further analysis to confirm.
