The galaxy presents as an elliptical or lenticular type, exhibiting a smooth, centrally concentrated light distribution. It appears largely featureless, with no readily discernible spiral arms or prominent dust lanes. The color profile suggests an older stellar population, with a yellowish-orange hue dominating the galaxy's overall appearance. There is no strong evidence of ongoing, significant star formation. The galaxy seems relatively isolated, without any obvious signs of tidal interactions or major disturbances to its structure, although there may be minor irregularities within the galactic halo. Its morphology is generally consistent with a galaxy that has undergone substantial evolution and is currently relatively quiescent.
