The galaxy presents a spiral morphology, exhibiting prominent spiral arms. These arms are well-defined and appear to be moderately wound. Two main spiral arms can be discerned. There is evidence of a central bulge with a moderate size relative to the disk. The disk component is easily visible. It is unlikely this is an edge on galaxy. It has no signs of being highly disturbed. The center of the galaxy appears to be dominated by older stars with a redder color. The spiral arms are a bit more blue, which indicates newer stars. There is not any strong evidence that this galaxy is merging.
