The galaxy appears to be a relatively smooth, elliptical system. It presents a centrally concentrated luminosity profile, exhibiting a diffuse, yellow-orange hue indicative of an older stellar population. There is no evident spiral structure or prominent dust lanes visible in this image. The galaxy has a near circular morphology. There is no evidence of tidal tails or strong morphological disturbances, suggesting the galaxy is relatively isolated and relaxed. Overall, the galaxy gives the impression of being an evolved, quiescent system.
