The galaxy presents as an elliptical or lenticular structure with a smooth, diffuse light distribution. The core exhibits a high degree of central concentration, transitioning outward to a fainter, more extended halo. There's a slight elongation along one axis, suggesting a moderate degree of ellipticity, but is close to being circular. No distinct spiral arms or prominent dust lanes are visible. The galaxy's color is generally yellowish. There are no signs of major interactions or recent merger events, although a minor disturbance cannot be ruled out. There is little evidence of active star formation, consistent with an older stellar population. The galaxy appears relatively isolated within its immediate vicinity.
