This galaxy exhibits a distinct spiral structure. Two prominent spiral arms emerge from a central bulge. These arms display a moderate winding, not tightly wound but also not fully open. Star formation appears to be active within the arms, indicated by the bluer hues intermixed with redder light, though the overall color index suggests a galaxy with an intermediate amount of ongoing star formation. The galaxy's bulge shows a moderate size relative to the disk. No obvious signs of a strong bar structure are apparent, nor any prominent tidal disturbances or evidence of a major merger event.
