The galaxy appears to be a relatively smooth, early-type spiral galaxy with a moderate redshift. It exhibits a noticeable central bulge, suggesting a concentration of older stars. The disk appears somewhat elongated, possibly cigar-shaped and is oriented at an angle relative to our line of sight. There are hints of subtle disturbances in its morphology. The light profile shows an overall smooth appearance and a very small amount of star formation is present. The galaxy is slightly elongated and does not show signs of a major merger event.
