The galaxy presents as a somewhat compact object with a moderate degree of central concentration. It has an overall smooth appearance, though subtle features suggest the possibility of a disk component or other irregularities. The galaxy's shape approximates a rounded form, showing no extreme elongation or bar structure. A slight color gradient is observed, with the central regions exhibiting a slightly yellower hue compared to the bluer outer regions. Based on its redshift, the galaxy is at an intermediate distance. Its estimated size is several kiloparsecs across. There is evidence for ongoing star formation, as the galaxy is neither a passive nor quiescent system. The overall morphology suggests it could be an early-type spiral galaxy or possibly an elliptical galaxy with some residual star formation activity. There is indication of interactions with other galaxies. 
