This galaxy appears to be a spiral galaxy, viewed at a slight angle relative to face-on. Spiral arms are visible, emanating from a moderately sized central bulge. These arms appear tightly wound close to the central bulge and extend outward. The color gradient suggests active star formation regions, with bluer hues tracing the spiral arms. The bulge exhibits a yellower/whiter tone, possibly indicating an older stellar population. The galaxy's disk is not perfectly smooth; there are some irregularities and hints of substructure, suggesting possible past interactions or ongoing accretion events. There is no prominent bar feature apparent. The disk shows some signs of disruption, but nothing to the point where it should be considered to be in a merger state. The galaxy seems to be undergoing spiral winding.
