The galaxy appears as a moderately bright, centrally concentrated object. It exhibits a roughly elliptical morphology. The core is a bright yellow and white, suggesting the presence of an older stellar population. Surrounding the core is a more diffuse region of light, with hints of blue which may suggest a younger population of stars. There is a subtle asymmetry in the outer regions, potentially hinting at minor gravitational interactions or disturbances. Overall, the galaxy presents a relatively smooth appearance, lacking prominent spiral arm structures or significant dust lanes. The galaxy does not show any visual evidence of an ongoing major merger.
