The galaxy presents an overall elliptical morphology, appearing somewhat flattened. It has a smooth, diffuse light distribution, with a centrally concentrated region that fades towards the outer edges. There is no apparent spiral structure or prominent dust lanes. The core of the galaxy exhibits a slightly reddish hue, potentially indicating an older stellar population. The outer regions show bluer tones, which may signify the presence of younger stars.

Based on its appearance, this galaxy may be undergoing minor gravitational disturbance.
