The galaxy presents an elongated, cigar-like morphology. Its light is primarily yellowish-white, suggesting an older stellar population, with some evidence of redder regions indicative of ongoing or recent star formation. The galaxy appears to be undergoing some form of interaction or disturbance, potentially a merger, as there is an irregular structure evident. The overall luminosity suggests a substantial stellar mass. The light profile indicates a fairly smooth central region, with some clumpy features throughout. The morphology is more akin to an elliptical or lenticular galaxy, possibly with tidal features.
