The galaxy presents a predominantly smooth morphology, with a concentrated central bulge. The overall shape appears to be transitioning from round to somewhat elliptical. There may be subtle indications of minor disturbances within the galaxy's structure, although no major distortions or merging events are immediately apparent. Color gradients suggest a population of older stars, consistent with a relatively low ongoing star formation rate. The galaxy's size, at a redshift of z=0.217, suggests that it is a fairly massive galaxy.
