The galaxy displays a prominent spiral structure with well-defined arms. There appear to be two dominant spiral arms that emanate from the central bulge. These arms are moderately wound. The central bulge exhibits a yellowish hue, possibly indicating an older stellar population. The spiral arms display a bluer color, suggesting the presence of younger, hotter stars and active star formation. The galaxy does not appear to be significantly disturbed, but there is some indication of minor asymmetry in the spiral arm structure, possibly indicating a minor interaction. The bulge is of moderate size relative to the overall disk. No strong bar feature is discernible.
