The galaxy presents an overall smooth morphology with a suggestion of being elongated or cigar-shaped in its structure. The light distribution is centrally concentrated, and the color gradients appear to be relatively smooth, with a brighter, possibly older stellar population dominating the central regions. There is no obvious indication of spiral arms or significant dust lanes, suggesting a later-type classification. There are hints of possible disturbances to the structure, but these are relatively minor. The primary light appears to be coming from an elliptical distribution.
