This galaxy appears to be a relatively smooth, lenticular or early-type spiral galaxy at a redshift of approximately 0.158. It exhibits a predominantly cigar-shaped morphology, appearing elongated with a high degree of central concentration. The color profile suggests a relatively passive star formation rate. The galaxy shows some indications of potential minor disturbances or interactions, although there is no dominant merging event currently in progress. The size suggests that it is a relatively small galaxy, with an estimated radius of just over 6 kpc.
