The galaxy appears to be an elliptical or lenticular type, exhibiting a generally smooth, rounded morphology. The central bulge is prominent and has a yellowish hue, suggesting an older stellar population. There is little evidence of spiral arms or significant dust lanes. A faint, diffuse extension is visible emanating from one side of the main galaxy body. This may be indicative of tidal interactions or a minor merger event. The galaxy overall presents a relatively undisturbed, relaxed appearance.
