The galaxy presents as a relatively smooth object, with a centrally concentrated brightness profile. It appears elliptical in shape, exhibiting a high degree of circularity. The core region displays a strong emission in the green and red bands, suggesting older stellar populations. There is a faint, diffuse halo surrounding the central region of the galaxy, with an absence of distinct spiral arm structures. The overall color of the galaxy appears to be leaning towards the redder end of the spectrum, indicating a dominant population of older stars. There appears to be a small possibility of some sort of minor disturbance from the overall smoothness and symmetry of the galaxy, but not indicative of any major ongoing merger events.
