The galaxy presents as a relatively smooth, elliptical-shaped structure. It exhibits a concentrated, bright central bulge that gradually diffuses outward into a fainter, more extended halo. The color profile suggests an older stellar population, indicated by the reddish-yellow hue dominating the galaxy's light. There is no prominent dust lane or spiral arm structure visible. The overall morphology indicates that it is likely an elliptical galaxy, potentially an E3 or E4 on the Hubble sequence, based on its apparent ellipticity. There are no immediately obvious signs of recent major merger activity, though a minor disturbance cannot be ruled out based on the faint outer edges.
