The galaxy presents as a moderately luminous, lenticular system at a redshift of approximately 0.184, suggesting a considerable distance. It exhibits a well-defined, smooth morphology with a highly elongated, cigar-shaped appearance, indicative of a potentially edge-on orientation relative to our line of sight. The central bulge appears somewhat concentrated, exhibiting a yellowish-white color. There is a possible faint disk component. There is some evidence of disturbance but is probably not undergoing a major merging event. The galaxy's star formation rate appears to be moderate. The mass estimate is around 10^10 solar masses. 
