The galaxy presents as an elliptical structure with a bright, concentrated central region indicative of a galactic nucleus. The overall morphology appears smooth with a slight elongation along one axis. The light profile gradually decreases from the center outwards with no obvious spiral arms or distinct features such as dust lanes or star-forming regions. Color gradients suggest a relatively homogenous stellar population across the galaxy's visible extent, with a subtle bluer halo surrounding the yellower nucleus. There's a slight asymmetry suggesting a possible past merger. Overall, the galaxy appears to be a fairly evolved, quiescent system.
