The galaxy presents as a centrally concentrated object with a smooth, fairly symmetrical profile. The light distribution is dominated by a bulge-like structure that fades gradually toward the outer regions.

The color appears generally consistent, with a slight reddening toward the core region which implies an older stellar population there compared to the outer regions. There is no clear evidence of spiral arm structures or significant dust lanes, but some faint diffuse structures might be disk features. These features are not very well pronounced however. There is no obvious evidence of any ongoing major merger events or strong tidal features, but the light appears slightly disturbed on the outer edge.
