The galaxy exhibits a non-distinct morphology, appearing largely smooth and elongated in shape. The central region presents a concentrated luminosity, possibly indicating a bulge or core component. A faint extension protrudes from the brighter core, giving the overall structure a cigar-like appearance. There is evidence of disturbance, with irregular light distribution. The object is approximately 9 kpc across, given its redshift of 0.18. Star formation is present, but overall specific star formation rate appears low, indicating a galaxy that is no longer forming stars at a very high rate.
