The galaxy presents as a relatively smooth, disk-like structure with a prominent central bulge. The object exhibits an elliptical morphology, tending toward an intermediate roundness. The central bulge is bright and concentrated, emitting a relatively blue light suggesting a population of young, hot stars or perhaps an active galactic nucleus. The disk component is less clearly defined but shows hints of spiral structure with faint, indistinct arms that trail away from the bulge. There are no obvious signs of a major merger event, though minor disturbances or interactions cannot be ruled out. The galaxy's color profile shows that is it most bright in the G,R and Z bands, suggesting some ongoing star formation. Overall, it appears to be a medium sized spiral galaxy at a moderate redshift.
