The galaxy presents as a spiral type, viewed at an angle somewhere between face-on and slightly inclined. Prominent spiral arm structures are visible. The arms appear somewhat flocculent, exhibiting a patchy distribution of star formation regions rather than a grand, sweeping design.

A central bulge is apparent, with a yellowish color indicative of an older stellar population. The disk component appears bluer, likely due to ongoing star formation. There's a possible, very subtle bar structure. No signs of major mergers or significant tidal disturbances are obvious in this image, though there appears to be a minor disturbance.
