The galaxy presents as a relatively smooth, elliptical morphology. It exhibits a concentrated central bulge, characterized by a bright, yellowish-white hue. The light from the bulge gradually fades as it extends outwards into a fainter, more diffuse halo. There is a slight elongation of the galaxy along a major axis, resulting in a somewhat flattened appearance. No distinct spiral arm structures or dust lanes are apparent within the visible spectrum, further supporting the classification as an elliptical galaxy. There are no signs of major disturbances or ongoing merger activity visible in this image. The overall color profile suggests an older stellar population, consistent with a low star formation rate.
