The galaxy presents as a luminous, elliptical structure, elongated along its major axis. Its core exhibits a high degree of central concentration, marked by a bright, yellowish-white hue indicative of an older stellar population. Moving outward from the nucleus, the luminosity gradually decreases, fading into a fainter, more diffuse halo. The galaxy displays some distortion or tidal features at its outer edges, hinting at possible gravitational interactions.
