The galaxy presents as a relatively smooth, elongated structure. Its morphology is suggestive of a galaxy undergoing or having completed the transition from a spiral to an elliptical type. There are no obvious spiral arms visible. The light distribution is centrally concentrated with a gradual fading towards the edges. The color appears predominantly yellowish-orange, indicating a stellar population dominated by older, redder stars, with correspondingly low levels of on-going star formation. The overall structure is not perfectly symmetrical, but is also not displaying evidence of any major ongoing merger.
