This galaxy appears to be a spiral galaxy, exhibiting a flattened disk structure. The central region is dominated by a bright, yellowish bulge, which suggests a significant population of older stars. Extending outward from the bulge are faint, blueish spiral arms. The spiral arms appear somewhat tightly wound around the central bulge, giving the galaxy a relatively ordered spiral structure. There are subtle variations in the density and luminosity along the spiral arms, possibly indicating areas of active star formation. The outer regions of the disk appear less defined and more diffuse. There does not appear to be any major disruption or signs of ongoing major mergers. There are no strong indications of a prominent bar feature.
