This galaxy appears to be a disk galaxy at an appreciable distance, evidenced by its redshift. The central bulge is luminous and exhibits a yellowish hue. The disk component appears to be moderately inclined relative to our line of sight. There is evidence of spiral arm structure, though it appears somewhat flocculent rather than grand design. The overall color gradient suggests ongoing star formation, with bluer regions indicative of younger stellar populations within the spiral arms. There may be some tidal disturbances present within the structure, suggestive of a past interaction with another galaxy.
