The galaxy presents a generally smooth and elongated morphology, suggestive of an elliptical or lenticular type. Its light profile appears concentrated towards the center, showing a bright, diffuse core that gradually fades outwards. The primary axis of elongation indicates a preferred direction, while the galaxy exhibits very little indication of a spiral arm structure or distinct features. The color distribution appears relatively uniform across the galaxy, hinting at a stellar population with limited ongoing star formation. There is faint blue tint to the outer regions, possibly indicative of a younger stellar population. Overall, the galaxy seems relatively undisturbed, displaying minimal signs of recent mergers or tidal interactions.
