The galaxy presents as a relatively well-defined spiral, viewed at a significant inclination. There is a central bulge with a concentrated luminosity. The spiral arms appear flocculent and somewhat patchy. The color gradient indicates potential active star formation regions within the disk, as suggested by the bluer hues in the spiral arms. The overall structure appears fairly regular, though there is a suggestion of minor tidal interaction with a small distortion or plume on one side. No obvious strong bar feature is noted.
