The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge that exhibits a yellowish hue, suggesting an older stellar population. A faint disk component may be present with traces of blue light, hinting at some ongoing star formation, even though the bulk of the galaxy seems quiescent. There are no obvious signs of significant disturbances or major mergers. The galaxy appears largely round with a slight deviation toward an elongated shape.
