The galaxy presents as a relatively smooth, elliptical-like structure with an overall elongated shape. Its core exhibits a bright, concentrated luminosity, transitioning to a slightly fainter and more diffuse outer region. A subtle color gradient is observed, with the core exhibiting a yellow to white hue, possibly indicating an older stellar population. The outer regions appear bluer, hinting at the presence of some younger stars. There is a lack of distinct spiral arm structures or prominent dust lanes. Minor asymmetries or disturbances are suggested in the galaxy's morphology, implying the possibility of past interaction or a minor merger event.
