This galaxy presents as a spiral galaxy with a prominent disk structure. The spiral arms are well-defined, exhibiting a loose winding pattern. The galaxy appears slightly disturbed with features indicative of a possible ongoing or recent merging event. There is a distinct bulge component, which appears moderate in size. Based on the color distribution, it appears to have active star formation regions, especially within the spiral arms. The galaxy has an inclination that provides a somewhat face-on view, enabling observation of its spiral structure. There is no obvious bar structure present.
