The galaxy appears to be a relatively smooth, centrally concentrated object. It exhibits a moderate ellipticity, appearing more round than elongated. There is a hint of a diffuse halo surrounding the brighter central region. No distinct spiral arms or bar structures are readily apparent in this image. The galaxy has a slightly yellowish hue, suggesting an older stellar population with relatively low levels of recent star formation. There is no evidence of any major ongoing mergers or tidal disturbances affecting the main body of the galaxy, although a slight asymmetry in the outer regions cannot be ruled out.
