The galaxy presents as a spiral type, viewed at an angle closer to face-on. The central bulge appears somewhat small, and less pronounced than the disk. Faint spiral arms are visible, exhibiting a rather loose winding pattern. Hints of a two-armed structure can be observed.  The blue color in the arms suggest active star formation. There are some signs of minor disturbances in the outer regions of the disk, though there does not seem to be any major interaction.  The central bulge seems to have less star formation based on its color, but is is also difficult to determine. There is some presence of dust that can be seen, but is not the most prominent characteristic. A slight hint of a bar structure is present, but it is not strongly defined.
