The galaxy appears to be a spiral galaxy, likely viewed at an angle between edge-on and face-on. There is a bright central bulge, seemingly elliptical in shape, which is possibly an indicator of an older stellar population. Surrounding the bulge is a disk, subtly visible, with a faint spiral arm structure, suggesting some ongoing star formation. The color profile indicates the presence of both older, redder stars in the bulge, and bluer, younger stars in the spiral arms. There are no clear signs of a recent major merger event, though there is a hint of some minor disturbances in the overall structure.
