The galaxy presents as a relatively smooth, concentrated object. Its overall morphology is elliptical, appearing slightly elongated rather than perfectly spherical. The core region is bright and concentrated. The light appears yellow, suggesting an older stellar population. A faint, diffuse halo surrounds the core, fading into the background. There may be some evidence of a tidal feature or minor disturbance, indicated by a faint, extended structure to one side, but this could also be an artifact of the imaging process. There is no visible spiral arm structure or significant dust lanes. The galaxy appears to be relatively isolated, with no immediately apparent signs of interaction with other galaxies. 
