The galaxy presents as a somewhat smooth, elongated structure. It exhibits a cigar-like shape and appears to be an edge-on galaxy. The central region is distinctly brighter and has an orange-red hue, suggesting an older stellar population and minimal active star formation. The outer regions fade into a dimmer, slightly bluer coloration, potentially indicating the presence of some younger stars or gas. There is no obvious evidence of a spiral arm structure or significant dust lanes. The morphology is generally undisturbed, with no prominent signs of recent merger activity.
