The galaxy appears as a centrally concentrated object, roughly elliptical in shape, with a smooth, diffuse light distribution. The core region is notably brighter and exhibits a yellowish-white hue, suggesting a population of older stars. There is a subtle color gradient outwards from the core, transitioning to a slightly redder tone in the outer regions. No distinct spiral arm structures or significant dust lanes are visible within the galaxy's morphology. The overall appearance suggests a relatively quiescent system with little ongoing star formation. The galaxy shows a largely undisturbed morphology, with no clear signs of tidal interactions or recent mergers, although a slight irregularity in its outskirts could indicate minor disturbances.
